detected,line,grp,source_name,other_name,beam,ra,dec,l,b,vlow,vup,fwhm,vpeak,vrange,rms,peak,units,int,ref,is_interf,major,minor,telescope_ref,ra_hms,dec_dms,date_txt,gc_flag,mjy_flag,rms_mjy_flag,bgps,dist,thermal,classi,peak_num,atlasgal,interf_ra,interf_dec,interf_l,interf_b,rms_num,image_descr,dist_parallax_num,dist_parallax,beam_copy,v_step,rms_approx_flag,telescope_conf,date_e,radec_interf,grpv, ,,,,,(arcsec),deg. (J2000),deg. (J2000),(deg.),(deg.),(km/s),(km/s),(km/s),(km/s),(km/s),(Jy),(Jy),,(Jy*km/s),,,,,,(J2000),(J2000),,,,,,(kpc),line mark,line mark,,,,,,,,,,(kpc),,(km/s),,,,,, 1,5(-1)->6(0)_A+,G358.460-0.393,G358.4603-0.3912,,15.0000000000,265.8615810,-30.4531280,358.4601600,-0.3910170,,,,1.3,,18.000,19.04 (0.28),2,20.47 (0.52),NGU22,1,,,NRAOVLA,+17 43 26.7794,-30 27 11.262,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,265.8615810,-30.4531280,358.4601600,-0.3910170,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G358.4601-0.3929, 1,5(-1)->6(0)_A+,G358.460-0.393,G358.4603-0.3933,,15.0000000000,265.8635400,-30.4540170,358.4602900,-0.3929210,,,,-7.34,,18.000,4.51 (0.09),2,5.24 (0.18),NGU22,1,,,NRAOVLA,+17 43 27.2495,-30 27 14.461,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,265.8635400,-30.4540170,358.4602900,-0.3929210,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G358.4601-0.3929, 1,5(-1)->6(0)_A+,G358.721-0.126,G358.7214-0.1259,,15.0000000000,265.7595020,-30.0917330,358.7213550,-0.1261450,,,,10.7,,18.000,1.73 (0.04),2,2.07 (0.08),NGU22,1,,,NRAOVLA,+17 43 2.2806,-30 05 30.239,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,265.7595020,-30.0917330,358.7213550,-0.1261450,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G358.7215-0.1262, 1,5(-1)->6(0)_A+,G358.809-0.085,G358.8082-0.0857,,15.0000000000,265.7723360,-29.9965260,358.8081860,-0.0855460,,,,-56.29,,18.000,4.53 (0.09),2,5.06 (0.17),NGU22,1,,,NRAOVLA,+17 43 5.3606,-29 59 47.494,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,265.7723360,-29.9965260,358.8081860,-0.0855460,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G358.8087-0.0854, 1,5(-1)->6(0)_A+,G358.841-0.737,G358.8409-0.7371,,15.0000000000,266.4345240,-30.3093220,358.8411800,-0.7371640,,,,-20.99,,18.000,4.82 (0.1),2,5.56 (0.21),NGU22,1,,,NRAOVLA,+17 45 44.2858,-30 18 33.56,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,266.4345240,-30.3093220,358.8411800,-0.7371640,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G358.8412-0.7372, 1,5(-1)->6(0)_A+,G358.906+0.106,G358.9047+0.1046,,15.0000000000,265.6438020,-29.8134410,358.9052630,0.1055310,,,,-18.12,,18.000,1.55 (0.03),2,1.81 (0.06),NGU22,1,,,NRAOVLA,+17 42 34.5125,-29 48 48.387,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,265.6438020,-29.8134410,358.9052630,0.1055310,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G358.9057+0.1056, 1,5(-1)->6(0)_A+,G358.931-0.030,G358.9304-0.0301,,15.0000000000,265.7917660,-29.8631060,358.9305430,-0.0297500,,,,-15.96,,18.000,5.47 (0.17),2,6.46 (0.33),NGU22,1,,,NRAOVLA,+17 43 10.0239,-29 51 47.18,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,265.7917660,-29.8631060,358.9305430,-0.0297500,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G358.9309-0.0295, 1,5(-1)->6(0)_A+,G358.386-0.479,G358.3865-0.4831,,15.0000000000,265.9076720,-30.5641700,358.3864740,-0.4830930,,,,-6,,18.000,3.29 (0.05),2,3.65 (0.1),NGU22,1,,,NRAOVLA,+17 43 37.8414,-30 33 51.013,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,265.9076720,-30.5641700,358.3864740,-0.4830930,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G358.3864-0.4827, 1,5(-1)->6(0)_A+,G359.137+0.031,G359.1375+0.0312,,15.0000000000,265.8572950,-29.6549160,359.1375810,0.0311970,,,,-3.73,,18.000,10.06 (0.28),2,11.13 (0.51),NGU22,1,,,NRAOVLA,+17 43 25.7507,-29 39 17.697,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,265.8572950,-29.6549160,359.1375810,0.0311970,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G359.1374+0.0315, 1,5(-1)->6(0)_A+,G359.4363-0.1033,G359.4361-0.1035,,15.0000000000,266.1692080,-29.4711150,359.4362720,-0.1036110,,,,-46.93,,18.000,53.84 (0.71),2,57.1 (1.34),NGU22,1,,,NRAOVLA,+17 44 40.6099,-29 28 16.015,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,266.1692080,-29.4711150,359.4362720,-0.1036110,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G359.4363-0.1035, 1,5(-1)->6(0)_A+,G359.4363-0.1033,G359.4361-0.1021,,15.0000000000,266.1674910,-29.4703490,359.4361430,-0.1019360,,,,-56.65,,18.000,0.99 (0.02),2,1.16 (0.05),NGU22,1,,,NRAOVLA,+17 44 40.1978,-29 28 13.257,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,266.1674910,-29.4703490,359.4361430,-0.1019360,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G359.4363-0.1035, 1,5(-1)->6(0)_A+,G359.615-0.243,G359.6146-0.2431,,15.0000000000,266.4129230,-29.3917790,359.6147180,-0.2432780,,,,19.33,,18.000,37.03 (0.64),2,40.5 (1.24),NGU22,1,,,NRAOVLA,+17 45 39.1016,-29 23 30.403,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,266.4129230,-29.3917790,359.6147180,-0.2432780,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G359.6148-0.2432, 1,5(-1)->6(0)_A+,G359.702-0.350,G359.7021-0.3507,,15.0000000000,266.5698250,-29.3731170,359.7018010,-0.3503150,,,,15.73,,18.000,0.61 (0.03),2,0.88 (0.08),NGU22,1,,,NRAOVLA,+17 46 16.7579,-29 22 23.223,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,266.5698250,-29.3731170,359.7018010,-0.3503150,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G359.7018-0.3503, 1,5(-1)->6(0)_A+,G359.970-0.457,G359.9694-0.4577,,15.0000000000,266.8339520,-29.1999650,359.9693580,-0.4574020,,,,22.93,,18.000,1.92 (0.03),2,1.99 (0.05),NGU22,1,,,NRAOVLA,+17 47 20.1484,-29 11 59.874,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,266.8339520,-29.1999650,359.9693580,-0.4574020,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G359.9697-0.4574, 1,5(-1)->6(0)_A+,G359.9384+0.1703,G359.9385+0.1703,,15.0000000000,266.2025880,-28.8999400,359.9384690,0.1700470,,,,-0.5,,18.000,0.34 (0.02),2,0.41 (0.05),NGU22,1,,,NRAOVLA,+17 44 48.6212,-28 53 59.784,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,266.2025880,-28.8999400,359.9384690,0.1700470,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G359.9385+0.1703, 1,5(-1)->6(0)_A+,G0.546-0.852,G0.5466-0.8519,,15.0000000000,267.5605620,-28.9085260,0.5464770,-0.8515570,,,,13.58,,18.000,115.24 (1.46),2,131.52 (2.79),NGU22,1,,,NRAOVLA,+17 50 14.5349,-28 54 30.693,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,267.5605620,-28.9085260,0.5464770,-0.8515570,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G0.5460-0.8521, 1,5(-1)->6(0)_A+,G0.6449-0.0420,G0.6452-0.0421,,15.0000000000,266.8278610,-28.4067520,0.6451160,-0.0419760,,,,49.54,,18.000,46.83 (2),2,55.02 (4.01),NGU22,1,,,NRAOVLA,+17 47 18.6866,-28 24 24.306,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,266.8278610,-28.4067520,0.6451160,-0.0419760,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G0.6449-0.0420, 1,5(-1)->6(0)_A+,G0.6573-0.0413,G0.6570-0.0414,,15.0000000000,266.8337640,-28.3960210,0.6569840,-0.0408590,,,,50.62,,18.000,5.14 (0.18),2,5.8 (0.35),NGU22,1,,,NRAOVLA,+17 47 20.1033,-28 23 45.675,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,266.8337640,-28.3960210,0.6569840,-0.0408590,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G0.6576-0.0413, 1,5(-1)->6(0)_A+,G0.6667-0.0344,G0.6653-0.0359,,15.0000000000,266.8337720,-28.3865300,0.6651060,-0.0359490,,,,60.34,,18.000,5.3 (0.19),2,5.32 (0.34),NGU22,1,,,NRAOVLA,+17 47 20.1052,-28 23 11.508,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,266.8337720,-28.3865300,0.6651060,-0.0359490,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G0.6667-0.0337, 1,5(-1)->6(0)_A+,G0.6667-0.0344,G0.6667-0.0289,,15.0000000000,266.8278930,-28.3815520,0.6666860,-0.0289470,,,,70.42,,18.000,51.67 (1.63),2,57.97 (3.19),NGU22,1,,,NRAOVLA,+17 47 18.6944,-28 22 53.586,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,266.8278930,-28.3815520,0.6666860,-0.0289470,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G0.6667-0.0337, 1,5(-1)->6(0)_A+,G0.6667-0.0344,G0.6667-0.0289,,15.0000000000,266.8278930,-28.3815510,0.6666870,-0.0289460,,,,72.22,,18.000,10.25 (0.29),2,11.41 (0.56),NGU22,1,,,NRAOVLA,+17 47 18.6943,-28 22 53.583,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,266.8278930,-28.3815510,0.6666870,-0.0289460,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G0.6667-0.0337, 1,5(-1)->6(0)_A+,G0.6667-0.0344,G0.6729-0.0317,,15.0000000000,266.8337580,-28.3777490,0.6726110,-0.0313910,,,,58.18,,18.000,7.27 (0.16),2,7.62 (0.29),NGU22,1,,,NRAOVLA,+17 47 20.102,-28 22 39.898,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,266.8337580,-28.3777490,0.6726110,-0.0313910,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G0.6667-0.0337, 1,5(-1)->6(0)_A+,G0.6948-0.0378,G0.6952-0.0379,,15.0000000000,266.8533770,-28.3616940,0.6952860,-0.0378430,,,,67.9,,18.000,25.36 (0.55),2,27.3 (1.03),NGU22,1,,,NRAOVLA,+17 47 24.8105,-28 21 42.098,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,266.8533770,-28.3616940,0.6952860,-0.0378430,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G0.6948-0.0378, 1,5(-1)->6(0)_A+,G0.8358+0.1844,G0.8361+0.1843,,15.0000000000,266.7202910,-28.1260730,0.8360240,0.1845430,,,,3.46,,18.000,2.45 (0.04),2,2.64 (0.07),NGU22,1,,,NRAOVLA,+17 46 52.8698,-28 07 33.862,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,266.7202910,-28.1260730,0.8360240,0.1845430,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G0.8358+0.1844, 1,5(-1)->6(0)_A+,G0.084-0.641,G0.0847-0.6421,,15.0000000000,267.0829720,-29.1966550,0.0845860,-0.6417610,,,,12.5,,18.000,0.26 (0.02),2,0.26 (0.04),NGU22,1,,,NRAOVLA,+17 48 19.9133,-29 11 47.958,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,267.0829720,-29.1966550,0.0845860,-0.6417610,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G0.0842-0.6415, 1,5(-1)->6(0)_A+,G0.3757+0.0400,G0.3759+0.0399,,15.0000000000,266.5888850,-28.5946850,0.3754910,0.0400470,,,,37,,18.000,0.1 (0.02),2,0.31 (0.07),NGU22,1,,,NRAOVLA,+17 46 21.3323,-28 35 40.866,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,266.5888850,-28.5946850,0.3754910,0.0400470,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G0.3758+0.0400, 1,5(-1)->6(0)_A+,G0.092-0.663,G0.0917-0.6630,,15.0000000000,267.1079740,-29.2012840,0.0918840,-0.6628450,,,,21.85,,18.000,11.64 (0.12),2,12.12 (0.23),NGU22,1,,,NRAOVLA,+17 48 25.9138,-29 12 4.623,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,267.1079740,-29.2012840,0.0918840,-0.6628450,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G0.0916-0.6630, 1,5(-1)->6(0)_A+,G0.4752-0.0096,G0.4755-0.0097,,15.0000000000,266.6962040,-28.5349380,0.4754990,-0.0094740,,,,27.98,,18.000,2.22 (0.05),2,2.46 (0.11),NGU22,1,,,NRAOVLA,+17 46 47.089,-28 32 5.776,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,266.6962040,-28.5349380,0.4754990,-0.0094740,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G0.4752-0.0096, 1,5(-1)->6(0)_A+,G0.6472-0.0551,G0.6472-0.0551,,15.0000000000,266.8421280,-28.4115360,0.6475240,-0.0551890,,,,50.98,,18.000,3.08 (0.12),2,3.54 (0.24),NGU22,1,,,NRAOVLA,+17 47 22.1108,-28 24 41.528,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,266.8421280,-28.4115360,0.6475240,-0.0551890,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G0.6472-0.0551, 1,5(-1)->6(0)_A+,G0.6512-0.0487,G0.6513-0.0488,,15.0000000000,266.8382160,-28.4047760,0.6515240,-0.0487440,,,,48.1,,18.000,14.24 (0.53),2,15.95 (1.02),NGU22,1,,,NRAOVLA,+17 47 21.1719,-28 24 17.193,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,266.8382160,-28.4047760,0.6515240,-0.0487440,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G0.6512-0.0487, 1,5(-1)->6(0)_A+,G0.6771-0.0269,G0.6771-0.0252,,15.0000000000,266.8304850,-28.3704540,0.6773600,-0.0251490,,,,73.3,,18.000,4.78 (0.12),2,4.99 (0.22),NGU22,1,,,NRAOVLA,+17 47 19.3165,-28 22 13.634,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,266.8304850,-28.3704540,0.6773600,-0.0251490,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G0.6667-0.0337, 1,5(-1)->6(0)_A+,G0.167-0.446,G0.1674-0.4456,,15.0000000000,266.9395040,-29.0244560,0.1672660,-0.4454740,,,,13.58,,18.000,1.26 (0.02),2,1.27 (0.03),NGU22,1,,,NRAOVLA,+17 47 45.4809,-29 01 28.043,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,266.9395040,-29.0244560,0.1672660,-0.4454740,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G0.1669-0.4456, 1,5(-1)->6(0)_A+,G0.212-0.517,G0.2116-0.5165,,15.0000000000,267.0353170,-29.0231830,0.2116590,-0.5165400,,,,7.1,,18.000,0.77 (0.02),2,0.79 (0.04),NGU22,1,,,NRAOVLA,+17 48 8.4761,-29 01 23.458,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,267.0353170,-29.0231830,0.2116590,-0.5165400,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G0.2117-0.5165, 1,5(-1)->6(0)_A+,G0.281-0.482,G0.2825-0.4791,,15.0000000000,267.0398730,-28.9435280,0.2819280,-0.4788120,,,,15.38,,18.000,0.34 (0.03),2,0.46 (0.07),NGU22,1,,,NRAOVLA,+17 48 9.5695,-28 56 36.7,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,267.0398730,-28.9435280,0.2819280,-0.4788120,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G0.2819-0.4788, 1,5(-1)->6(0)_A+,G0.2118-0.0009,G0.2118+0.0002,,15.0000000000,266.5318370,-28.7555940,0.2120180,-0.0008570,,,,49.54,,18.000,2.89 (0.07),2,3.05 (0.13),NGU22,1,,,NRAOVLA,+17 46 7.6409,-28 45 20.137,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,266.5318370,-28.7555940,0.2120180,-0.0008570,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G0.2118-0.0009, 1,5(-1)->6(0)_A+,G0.315-0.201,G0.3160-0.2011,,15.0000000000,266.7883170,-28.7708100,0.3157470,-0.2009130,,,,18.26,,18.000,63.75 (1.85),2,70.72 (3.6),NGU22,1,,,NRAOVLA,+17 47 9.1961,-28 46 14.916,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,266.7883170,-28.7708100,0.3157470,-0.2009130,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G0.3154-0.2008, 1,5(-1)->6(0)_A+,G0.315-0.201,G0.3167-0.2011,,15.0000000000,266.7884030,-28.7704540,0.3160910,-0.2007930,,,,26.16,,18.000,0.74 (0.04),2,1.02 (0.09),NGU22,1,,,NRAOVLA,+17 47 9.2168,-28 46 13.634,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,266.7884030,-28.7704540,0.3160910,-0.2007930,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G0.3154-0.2008, 1,5(-1)->6(0)_A+,G0.4964+0.1880,G0.4965+0.1877,,15.0000000000,266.5165520,-28.4143970,0.4964400,0.1880860,,,,0.94,,18.000,23.77 (0.61),2,26.43 (1.14),NGU22,1,,,NRAOVLA,+17 46 3.9725,-28 24 51.831,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,266.5165520,-28.4143970,0.4964400,0.1880860,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G0.4964+0.1880, 1,5(-1)->6(0)_A+,G0.5069+0.1716,G0.5071+0.1718,,15.0000000000,266.5387180,-28.4140360,0.5068890,0.1716230,,,,-9.5,,18.000,0.31 (0.03),2,0.31 (0.05),NGU22,1,,,NRAOVLA,+17 46 9.2924,-28 24 50.529,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,266.5387180,-28.4140360,0.5068890,0.1716230,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G0.5069+0.1716, 1,5(-1)->6(0)_A+,G1.008-0.237,G1.0078-0.2371,,15.0000000000,267.2302160,-28.1967710,1.0079140,-0.2368320,,,,1.66,,18.000,7.86 (0.15),2,8.17 (0.27),NGU22,1,,,NRAOVLA,+17 48 55.2518,-28 11 48.377,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,267.2302160,-28.1967710,1.0079140,-0.2368320,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G1.0080-0.2369, 1,5(-1)->6(0)_A+,G1.1468-0.1245,G1.1466-0.1246,,15.0000000000,267.2022120,-28.0198170,1.1468420,-0.1244830,,,,-15.24,,18.000,5.1 (0.03),2,5.23 (0.05),NGU22,1,,,NRAOVLA,+17 48 48.5309,-28 01 11.342,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,267.2022120,-28.0198170,1.1468420,-0.1244830,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G1.1468-0.1245, 1,5(-1)->6(0)_A+,G1.719-0.088,G1.7175-0.0878,,15.0000000000,267.4992560,-27.5101590,1.7191090,-0.0877530,,,,-8.05,,18.000,1.98 (0.03),2,1.98 (0.05),NGU22,1,,,NRAOVLA,+17 49 59.8214,-27 30 36.572,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,267.4992560,-27.5101590,1.7191090,-0.0877530,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G1.7191-0.0879, 1,5(-1)->6(0)_A+,G1.2821-0.0840,G1.2821-0.0844,,15.0000000000,267.2417520,-27.8830930,1.2820170,-0.0839720,,,,-9.84,,18.000,1.03 (0.02),2,1.08 (0.03),NGU22,1,,,NRAOVLA,+17 48 58.0205,-27 52 59.134,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,267.2417520,-27.8830930,1.2820170,-0.0839720,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G1.2821-0.0840, 1,5(-1)->6(0)_A+,G1.3290+0.1496,G1.3290+0.1495,,15.0000000000,267.0429510,-27.7226870,1.3287360,0.1494180,,,,-12,,18.000,0.51 (0.02),2,0.53 (0.03),NGU22,1,,,NRAOVLA,+17 48 10.3083,-27 43 21.672,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,267.0429510,-27.7226870,1.3287360,0.1494180,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G1.3286+0.1496, 1,5(-1)->6(0)_A+,G1.3320+0.0915,G1.3325+0.0911,,15.0000000000,267.1009080,-27.7497580,1.3320360,0.0915100,,,,-6.6,,18.000,0.14 (0.02),2,0.28 (0.05),NGU22,1,,,NRAOVLA,+17 48 24.2178,-27 44 59.129,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,267.1009080,-27.7497580,1.3320360,0.0915100,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G1.3320+0.0915, 1,5(-1)->6(0)_A+,G1.6785-0.1250,G1.6790-0.1256,,15.0000000000,267.5118250,-27.5640830,1.6785500,-0.1249960,,,,42,,18.000,0.2 (0.02),2,0.18 (0.02),NGU22,1,,,NRAOVLA,+17 50 2.8379,-27 33 50.7,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,267.5118250,-27.5640830,1.6785500,-0.1249960,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G1.6785-0.1250, 1,5(-1)->6(0)_A+,G1.4342-0.0021,G1.4346-0.0025,,15.0000000000,267.2510480,-27.7104940,1.4341960,-0.0021200,,,,13.2,,18.000,0.82 (0.02),2,0.88 (0.03),NGU22,1,,,NRAOVLA,+17 49 0.2516,-27 42 37.777,Dec 2011 - Apr 2017,1,0,1,,,0,0,,,267.2510480,-27.7104940,1.4341960,-0.0021200,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G1.4342-0.0021, 1,5(-1)->6(0)_A+,G2.521-0.220,G2.5210-0.2205,,15.0000000000,268.0880540,-26.8889760,2.5207180,-0.2201920,,,,-5.71,,18.000,1.12 (0.01),2,1.12 (0.02),NGU22,1,,,NRAOVLA,+17 52 21.1329,-26 53 20.313,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,268.0880540,-26.8889760,2.5207180,-0.2201920,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G2.5207-0.2203, 1,5(-1)->6(0)_A+,G2.591-0.029,G2.5919-0.0296,,15.0000000000,267.9444090,-26.7307110,2.5915140,-0.0292150,,,,-7.87,,18.000,1.12 (0.01),2,1.14 (0.03),NGU22,1,,,NRAOVLA,+17 51 46.6581,-26 43 50.558,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,267.9444090,-26.7307110,2.5915140,-0.0292150,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G2.5914-0.0294, 1,5(-1)->6(0)_A+,G2.143+0.009,G2.1433+0.0086,,15.0000000000,267.6504670,-27.0965410,2.1431050,0.0089970,,,,59.48,,18.000,6.22 (0.08),2,6.39 (0.14),NGU22,1,,,NRAOVLA,+17 50 36.1121,-27 05 47.547,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,267.6504670,-27.0965410,2.1431050,0.0089970,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G2.1432+0.0090, 1,5(-1)->6(0)_A+,G2.304+0.239,G2.3030+0.2593,,15.0000000000,267.5013290,-26.8307970,2.3030870,0.2593870,,,,9.8,,18.000,1.21 (0.02),2,1.23 (0.03),NGU22,1,,,NRAOVLA,+17 50 0.3189,-26 49 50.871,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,267.5013290,-26.8307970,2.3030870,0.2593870,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G2.3031+0.2594, 1,5(-1)->6(0)_A+,G2.536+0.198,G2.5356+0.1982,,15.0000000000,267.6936500,-26.6626580,2.5354960,0.1981210,,,,6.21,,18.000,11.98 (0.08),2,12.05 (0.13),NGU22,1,,,NRAOVLA,+17 50 46.4759,-26 39 45.569,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,267.6936500,-26.6626580,2.5354960,0.1981210,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G2.5355+0.1982, 1,5(-1)->6(0)_A+,G2.615+0.134,G2.6155+0.1336,,15.0000000000,267.8011240,-26.6268070,2.6154470,0.1339260,,,,94.05,,18.000,0.92 (0.01),2,0.94 (0.02),NGU22,1,,,NRAOVLA,+17 51 12.2698,-26 37 36.504,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,267.8011240,-26.6268070,2.6154470,0.1339260,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G2.6153+0.1339, 1,5(-1)->6(0)_A+,G2.703+0.042,G2.7037+0.0399,,15.0000000000,267.9415030,-26.5990300,2.7034340,0.0402150,,,,95.13,,18.000,9.57 (0.08),2,9.57 (0.14),NGU22,1,,,NRAOVLA,+17 51 45.9607,-26 35 56.507,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,267.9415030,-26.5990300,2.7034340,0.0402150,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G2.7034+0.0402, 1,5(-1)->6(0)_A+,G3.312-0.399,G3.3120-0.3986,,15.0000000000,268.7084190,-26.2968910,3.3123750,-0.3979280,,,,0.5,,18.000,0.42 (0.01),2,0.46 (0.03),NGU22,1,,,NRAOVLA,+17 54 50.0206,-26 17 48.808,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,268.7084190,-26.2968910,3.3123750,-0.3979280,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G3.3119-0.3986, 1,5(-1)->6(0)_A+,G3.442-0.348,G3.4422-0.3484,,15.0000000000,268.7339400,-26.1600900,3.4420080,-0.3485850,,,,-35,,18.000,0.32 (0.01),2,0.4 (0.03),NGU22,1,,,NRAOVLA,+17 54 56.1457,-26 09 36.323,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,268.7339400,-26.1600900,3.4420080,-0.3485850,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G3.4421-0.3485, 1,5(-1)->6(0)_A+,G3.253+0.018,G3.2536+0.0183,,15.0000000000,268.2747270,-26.1369780,3.2531210,0.0185350,,,,2.38,,18.000,3.37 (0.03),2,3.46 (0.05),NGU22,1,,,NRAOVLA,+17 53 5.9346,-26 08 13.121,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,268.2747270,-26.1369780,3.2531210,0.0185350,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G3.2532+0.0185, 1,5(-1)->6(0)_A+,G3.910+0.001,G3.9105+0.0009,,15.0000000000,268.6615260,-25.5791710,3.9103880,0.0011780,,,,17.53,,18.000,4.58 (0.02),2,4.6 (0.04),NGU22,1,,,NRAOVLA,+17 54 38.7663,-25 34 45.017,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,268.6615260,-25.5791710,3.9103880,0.0011780,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G3.9104+0.0012, 1,5(-1)->6(0)_A+,G3.502-0.200,G3.5022-0.2005,,15.0000000000,268.6251460,-26.0333170,3.5020180,-0.2002070,,,,43.79,,18.000,0.65 (0.01),2,0.66 (0.03),NGU22,1,,,NRAOVLA,+17 54 30.0351,-26 01 59.943,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,268.6251460,-26.0333170,3.5020180,-0.2002070,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G3.5022-0.2002, 1,5(-1)->6(0)_A+,G3.427-0.146,G3.4272-0.1456,,15.0000000000,268.5307530,-26.0704760,3.4270530,-0.1458710,,,,17.89,,18.000,0.67 (0.02),2,0.7 (0.03),NGU22,1,,,NRAOVLA,+17 54 7.3808,-26 04 13.712,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,268.5307530,-26.0704760,3.4270530,-0.1458710,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G3.4271-0.1459, 1,5(-1)->6(0)_A+,G3.347-0.076,G3.3514-0.0779,,15.0000000000,268.4225180,-26.1013330,3.3511900,-0.0777040,,,,4.54,,18.000,0.37 (0.02),2,0.41 (0.05),NGU22,1,,,NRAOVLA,+17 53 41.4044,-26 06 4.797,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,268.4225180,-26.1013330,3.3511900,-0.0777040,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G3.3505-0.0787, 1,5(-1)->6(0)_A+,G4.824-0.081,G4.8253-0.0816,,15.0000000000,269.2489380,-24.8311660,4.8242740,-0.0812390,,,,22.56,,18.000,0.26 (0.01),2,0.32 (0.03),NGU22,1,,,NRAOVLA,+17 56 59.7452,-24 49 52.199,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,269.2489380,-24.8311660,4.8242740,-0.0812390,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G4.8243-0.0812, 1,5(-1)->6(0)_A+,G4.434+0.129,G4.4344+0.1289,,15.0000000000,268.8322900,-25.0622810,4.4344790,0.1289700,,,,-0.9,,18.000,0.58 (0.01),2,0.63 (0.03),NGU22,1,,,NRAOVLA,+17 55 19.7497,-25 03 44.21,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,268.8322900,-25.0622810,4.4344790,0.1289700,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G4.4343+0.1289, 1,5(-1)->6(0)_A+,G4.416+0.123,G4.4160+0.1266,,15.0000000000,268.8239270,-25.0796010,4.4157020,0.1267740,,,,0.18,,18.000,0.58 (0.01),2,0.59 (0.03),NGU22,1,,,NRAOVLA,+17 55 17.7424,-25 04 46.565,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,268.8239270,-25.0796010,4.4157020,0.1267740,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G4.4157+0.1268, 1,5(-1)->6(0)_A+,G4.569-0.079,G4.5689-0.0791,,15.0000000000,269.1053860,-25.0510900,4.5687260,-0.0791340,,,,9.5,,18.000,0.7 (0.01),2,0.72 (0.02),NGU22,1,,,NRAOVLA,+17 56 25.2927,-25 03 3.923,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,269.1053860,-25.0510900,4.5687260,-0.0791340,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G4.5688-0.0791, 1,5(-1)->6(0)_A+,G4.866-0.171,G4.8663-0.1715,,15.0000000000,269.3584970,-24.8398510,4.8666150,-0.1716170,,,,5.4,,18.000,0.26 (0.01),2,0.29 (0.02),NGU22,1,,,NRAOVLA,+17 57 26.0392,-24 50 23.464,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,269.3584970,-24.8398510,4.8666150,-0.1716170,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G4.8662-0.1715, 1,5(-1)->6(0)_A+,G4.393+0.079,G4.3940+0.0784,,15.0000000000,268.8572650,-25.1228990,4.3935420,0.0788670,,,,2.02,,18.000,6.32 (0.03),2,6.2 (0.06),NGU22,1,,,NRAOVLA,+17 55 25.7436,-25 07 22.438,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,268.8572650,-25.1228990,4.3935420,0.0788670,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G4.3933+0.0786, 1,5(-1)->6(0)_A+,G4.586+0.028,G4.5863+0.0278,,15.0000000000,269.0134350,-24.9820970,4.5864460,0.0275860,,,,25.81,,18.000,0.32 (0.01),2,0.29 (0.03),NGU22,1,,,NRAOVLA,+17 56 3.2245,-24 58 55.548,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,269.0134350,-24.9820970,4.5864460,0.0275860,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G4.5864+0.0275, 1,5(-1)->6(0)_A+,G4.676+0.276,G4.6766+0.2764,,15.0000000000,268.8263420,-24.7791530,4.6762240,0.2764500,,,,4.54,,18.000,2.11 (0.01),2,2.07 (0.03),NGU22,1,,,NRAOVLA,+17 55 18.3221,-24 46 44.952,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,268.8263420,-24.7791530,4.6762240,0.2764500,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G4.6762+0.2764, 1,5(-1)->6(0)_A+,G5.587-0.252,G5.5870-0.2520,,15.0000000000,269.8303230,-24.2557620,5.5870090,-0.2515700,,,,0.31,,18.000,0.4 (0.02),2,0.42 (0.04),NGU22,1,,,NRAOVLA,+17 59 19.2774,-24 15 20.744,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,269.8303230,-24.2557620,5.5870090,-0.2515700,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G5.5870-0.2516, 1,5(-1)->6(0)_A+,G5.043-0.099,G5.0425-0.0978,,15.0000000000,269.3851430,-24.6508230,5.0423330,-0.0978560,,,,44.19,,18.000,0.56 (0.03),2,0.46 (0.04),NGU22,1,,,NRAOVLA,+17 57 32.4343,-24 39 2.961,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,269.3851430,-24.6508230,5.0423330,-0.0978560,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G5.0426-0.0985, 1,5(-1)->6(0)_A+,G5.900-0.430,G5.9002-0.4298,,15.0000000000,270.1702540,-24.0724980,5.9002090,-0.4295720,,,,9.62,,18.000,2.41 (0.03),2,2.43 (0.06),NGU22,1,,,NRAOVLA,+18 00 40.8609,-24 04 20.992,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,270.1702540,-24.0724980,5.9002090,-0.4295720,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G5.9003-0.4292, 1,5(-1)->6(0)_A+,G5.885-0.392,G5.8849-0.3937,,15.0000000000,270.1275090,-24.0675190,5.8851650,-0.3932180,,,,6.79,,18.000,0.73 (0.03),2,0.75 (0.06),NGU22,1,,,NRAOVLA,+18 00 30.6021,-24 04 3.069,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,270.1275090,-24.0675190,5.8851650,-0.3932180,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G5.8852-0.3923, 1,5(-1)->6(0)_A+,G5.677-0.027,G5.6773-0.0277,,15.0000000000,269.6664690,-24.0657380,5.6771690,-0.0272250,,,,-11.64,,18.000,0.43 (0.02),2,0.43 (0.03),NGU22,1,,,NRAOVLA,+17 58 39.9526,-24 03 56.658,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,269.6664690,-24.0657380,5.6771690,-0.0272250,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G5.6771-0.0273, 1,5(-1)->6(0)_A+,G5.657+0.416,G5.6571+0.4161,,15.0000000000,269.2354750,-23.8613910,5.6569580,0.4160160,,,,19.42,,18.000,2.77 (0.02),2,2.82 (0.04),NGU22,1,,,NRAOVLA,+17 56 56.514,-23 51 41.006,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,269.2354750,-23.8613910,5.6569580,0.4160160,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G5.6569+0.4159, 1,5(-1)->6(0)_A+,G5.630-0.294,G5.6300-0.2943,,15.0000000000,269.8941880,-24.2398010,5.6298480,-0.2941190,,,,9.98,,18.000,1.27 (0.03),2,1.32 (0.05),NGU22,1,,,NRAOVLA,+17 59 34.6051,-24 14 23.283,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,269.8941880,-24.2398010,5.6298480,-0.2941190,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G5.6297-0.2941, 1,5(-1)->6(0)_A+,G5.618-0.082,G5.6182-0.0825,,15.0000000000,269.6865370,-24.1444160,5.6181340,-0.0823670,,,,-26.39,,18.000,2.54 (0.02),2,2.58 (0.04),NGU22,1,,,NRAOVLA,+17 58 44.7689,-24 08 39.898,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,269.6865370,-24.1444160,5.6181340,-0.0823670,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G5.6181-0.0824, 1,5(-1)->6(0)_A+,G6.368-0.051,G6.3680-0.0522,,15.0000000000,270.0659380,-23.4788760,6.3681370,-0.0520170,,,,144.05,,18.000,1.86 (0.03),2,1.86 (0.05),NGU22,1,,,NRAOVLA,+18 00 15.8252,-23 28 43.952,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,270.0659380,-23.4788760,6.3681370,-0.0520170,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G6.3682-0.0520, 1,5(-1)->6(0)_A+,G6.189-0.358,G6.1886-0.3585,,15.0000000000,270.2590010,-23.7863540,6.1889300,-0.3581410,,,,-30.25,,18.000,232.36 (1.75),2,235.11 (3.18),NGU22,1,,,NRAOVLA,+18 01 2.1602,-23 47 10.876,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,270.2590010,-23.7863540,6.1889300,-0.3581410,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G6.1890-0.3582, 1,5(-1)->6(0)_A+,G6.226-0.053,G6.2297-0.0574,,15.0000000000,269.9956750,-23.6018650,6.2293980,-0.0572390,,,,19.43,,18.000,1.18 (0.03),2,1.16 (0.05),NGU22,1,,,NRAOVLA,+17 59 58.9619,-23 36 6.715,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,269.9956750,-23.6018650,6.2293980,-0.0572390,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G6.2294-0.0572, 1,5(-1)->6(0)_A+,G6.881+0.093,G6.8809+0.0929,,15.0000000000,270.2057240,-22.9617610,6.8808210,0.0931210,,,,-2.15,,18.000,3.68 (0.02),2,3.85 (0.04),NGU22,1,,,NRAOVLA,+18 00 49.3737,-22 57 42.339,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,270.2057240,-22.9617610,6.8808210,0.0931210,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G6.8808+0.0931, 1,5(-1)->6(0)_A+,G6.794-0.256,G6.7955-0.2571,,15.0000000000,270.4905700,-23.2093290,6.7954460,-0.2571120,,,,25.92,,18.000,38.19 (0.25),2,38.72 (0.45),NGU22,1,,,NRAOVLA,+18 01 57.7368,-23 12 33.583,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,270.4905700,-23.2093290,6.7954460,-0.2571120,0.018,,,,,0.18,1,D,,,G6.7937-0.2558, 1,5(-1)->6(0)_A+,G6.610-0.082,G6.6101-0.0821,,15.0000000000,270.2250890,-23.2838070,6.6099860,-0.0820330,,,,0.72,,18.000,22.17 (0.12),2,22.48 (0.22),NGU22,1,,,NRAOVLA,+18 00 54.0213,-23 17 1.705,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,270.2250890,-23.2838070,6.6099860,-0.0820330,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G6.6099-0.0823, 1,5(-1)->6(0)_A+,G6.610-0.082,G6.6070-0.0896,,15.0000000000,270.2304660,-23.2903950,6.6067130,-0.0895890,,,,9.72,,18.000,1.01 (0.02),2,1.05 (0.04),NGU22,1,,,NRAOVLA,+18 00 55.3118,-23 17 25.423,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,270.2304660,-23.2903950,6.6067130,-0.0895890,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G6.6067-0.0896, 1,5(-1)->6(0)_A+,G6.588-0.192,G6.5879-0.1918,,15.0000000000,270.3170000,-23.3573620,6.5879190,-0.1917930,,,,5.04,,18.000,7.95 (0.08),2,8.03 (0.15),NGU22,1,,,NRAOVLA,+18 01 16.0801,-23 21 26.503,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,270.3170000,-23.3573620,6.5879190,-0.1917930,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G6.5879-0.1919, 1,5(-1)->6(0)_A+,G6.545-0.270,G6.5453-0.2695,,15.0000000000,270.3675760,-23.4330560,6.5451340,-0.2695980,,,,22.86,,18.000,0.53 (0.02),2,0.64 (0.04),NGU22,1,,,NRAOVLA,+18 01 28.2182,-23 25 59,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,270.3675760,-23.4330560,6.5451340,-0.2695980,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G6.5451-0.2696, 1,5(-1)->6(0)_A+,G6.509-0.202,G6.5091-0.2016,,15.0000000000,270.2837230,-23.4307460,6.5090410,-0.2016120,,,,1.26,,18.000,0.3 (0.02),2,0.36 (0.05),NGU22,1,,,NRAOVLA,+18 01 8.0936,-23 25 50.687,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,270.2837230,-23.4307460,6.5090410,-0.2016120,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G6.5090-0.2016, 1,5(-1)->6(0)_A+,G6.551-0.098,G6.5393-0.1085,,15.0000000000,270.2117650,-23.3580750,6.5394230,-0.1082330,,,,12.91,,18.000,0.55 (0.02),2,0.54 (0.04),NGU22,1,,,NRAOVLA,+18 00 50.8237,-23 21 29.07,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,270.2117650,-23.3580750,6.5394230,-0.1082330,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G6.5393-0.1085, 1,5(-1)->6(0)_A+,G7.635-0.193,G7.6354-0.1923,,15.0000000000,270.8785560,-22.4470840,7.6349140,-0.1923520,,,,146.03,,18.000,0.79 (0.02),2,0.82 (0.04),NGU22,1,,,NRAOVLA,+18 03 30.8534,-22 26 49.501,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,270.8785560,-22.4470840,7.6349140,-0.1923520,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G7.6355-0.1932, 1,5(-1)->6(0)_A+,G7.166+0.131,G7.1659+0.1313,,15.0000000000,270.3229000,-22.6956910,7.1654430,0.1311720,,,,85.61,,18.000,3.09 (0.02),2,3.15 (0.03),NGU22,1,,,NRAOVLA,+18 01 17.4961,-22 41 44.486,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,270.3229000,-22.6956910,7.1654430,0.1311720,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G7.1655+0.1313, 1,5(-1)->6(0)_A+,G7.166+0.131,G7.1659+0.1313,,15.0000000000,270.3229000,-22.6956920,7.1654420,0.1311710,,,,74.81,,18.000,1.71 (0.02),2,1.81 (0.03),NGU22,1,,,NRAOVLA,+18 01 17.496,-22 41 44.49,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,270.3229000,-22.6956920,7.1654420,0.1311710,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G7.1655+0.1313, 1,5(-1)->6(0)_A+,G7.601-0.139,G7.6014-0.1388,,15.0000000000,270.8101930,-22.4503710,7.6009550,-0.1389690,,,,152.14,,18.000,4.71 (0.03),2,4.77 (0.06),NGU22,1,,,NRAOVLA,+18 03 14.4462,-22 27 1.335,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,270.8101930,-22.4503710,7.6009550,-0.1389690,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G7.6010-0.1389, 1,5(-1)->6(0)_A+,G7.632-0.109,G7.6319-0.1089,,15.0000000000,270.7984520,-22.4091410,7.6314960,-0.1092220,,,,156.91,,18.000,4.78 (0.04),2,4.94 (0.08),NGU22,1,,,NRAOVLA,+18 03 11.6284,-22 24 32.908,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,270.7984520,-22.4091410,7.6314960,-0.1092220,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G7.6316-0.1092, 1,5(-1)->6(0)_A+,G8.139+0.226,G8.1412+0.2263,,15.0000000000,270.7530990,-21.8026560,8.1386050,0.2260850,,,,19.92,,18.000,3.91 (0.03),2,3.83 (0.06),NGU22,1,,,NRAOVLA,+18 03 0.7437,-21 48 9.562,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,270.7530990,-21.8026560,8.1386050,0.2260850,0.018,,,,,0.18,1,D,,,G8.1386+0.2260, 1,5(-1)->6(0)_A+,G8.317-0.096,G8.3176-0.0960,,15.0000000000,271.1500990,-21.8054390,8.3173750,-0.0962720,,,,46.63,,18.000,2.92 (0.02),2,2.95 (0.04),NGU22,1,,,NRAOVLA,+18 04 36.0238,-21 48 19.58,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,271.1500990,-21.8054390,8.3173750,-0.0962720,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G8.3174-0.0963, 1,5(-1)->6(0)_A+,G8.669-0.357,G8.6697-0.3557,,15.0000000000,271.5790340,-21.6254520,8.6693160,-0.3557570,,,,39.44,,18.000,4.05 (0.03),2,4.19 (0.06),NGU22,1,,,NRAOVLA,+18 06 18.9681,-21 37 31.627,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,271.5790340,-21.6254520,8.6693160,-0.3557570,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G8.6692-0.3560, 1,5(-1)->6(0)_A+,G8.669-0.357,G8.6829-0.3682,,15.0000000000,271.5976900,-21.6194520,8.6830170,-0.3679670,,,,43.12,,18.000,135.04 (0.47),2,135.68 (0.85),NGU22,1,,,NRAOVLA,+18 06 23.4457,-21 37 10.028,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,271.5976900,-21.6194520,8.6830170,-0.3679670,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G8.6831-0.3680, 1,5(-1)->6(0)_A+,G8.832-0.028,G8.8315-0.0279,,15.0000000000,271.3568740,-21.3236900,8.8315640,-0.0279210,,,,-3.95,,18.000,136.3 (1.19),2,138.54 (2.15),NGU22,1,,,NRAOVLA,+18 05 25.6498,-21 19 25.285,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,271.3568740,-21.3236900,8.8315640,-0.0279210,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G8.8316-0.0280, 1,5(-1)->6(0)_A+,G8.872-0.493,G8.8725-0.4932,,15.0000000000,271.8140240,-21.5149270,8.8723440,-0.4927030,,,,23.25,,18.000,45.07 (0.43),2,46.04 (0.79),NGU22,1,,,NRAOVLA,+18 07 15.3657,-21 30 53.739,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,271.8140240,-21.5149270,8.8723440,-0.4927030,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G8.8723-0.4927, 1,5(-1)->6(0)_A+,G8.222+0.562,G8.2225+0.5617,,15.0000000000,270.4833890,-21.5640930,8.2224320,0.5617910,,,,13.95,,18.000,0.66 (0.02),2,0.65 (0.03),NGU22,1,,,NRAOVLA,+18 01 56.0134,-21 33 50.736,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,270.4833890,-21.5640930,8.2224320,0.5617910,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G8.2224+0.5618, 1,5(-1)->6(0)_A+,G9.215-0.202,G9.2145-0.2018,,15.0000000000,271.7201200,-21.0742150,9.2146470,-0.2016440,,,,41.64,,18.000,5.7 (0.04),2,5.85 (0.07),NGU22,1,,,NRAOVLA,+18 06 52.8289,-21 04 27.173,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,271.7201200,-21.0742150,9.2146470,-0.2016440,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G9.2146-0.2017, 1,5(-1)->6(0)_A+,G9.621+0.195,G9.6211+0.1956,,15.0000000000,271.5610450,-20.5251070,9.6214770,0.1960020,,,,-88.72,,18.000,1.14 (0.04),2,1.14 (0.08),NGU22,1,,,NRAOVLA,+18 06 14.6509,-20 31 30.386,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,271.5610450,-20.5251070,9.6214770,0.1960020,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G9.6209+0.1952, 1,5(-1)->6(0)_A+,G9.621+0.195,G9.6213+0.1961,,15.0000000000,271.5610410,-20.5251940,9.6214000,0.1959640,,,,1.3,,18.000,5412.52 (79.17),2,5744.23 (147.02),NGU22,1,,,NRAOVLA,+18 06 14.6498,-20 31 30.698,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,271.5610410,-20.5251940,9.6214000,0.1959640,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G9.6209+0.1952, 1,5(-1)->6(0)_A+,G9.621+0.195,G9.6187+0.1932,,15.0000000000,271.5621550,-20.5284850,9.6190370,0.1934470,,,,5.4,,18.000,48.39 (1.7),2,58.76 (3.45),NGU22,1,,,NRAOVLA,+18 06 14.9171,-20 31 42.545,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,271.5621550,-20.5284850,9.6190370,0.1934470,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G9.6209+0.1952, 1,5(-1)->6(0)_A+,G9.986-0.030,G9.9862-0.0273,,15.0000000000,271.9587600,-20.3157120,9.9859080,-0.0275110,,,,42.27,,18.000,69.6 (0.6),2,72.78 (1.09),NGU22,1,,,NRAOVLA,+18 07 50.1023,-20 18 56.562,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,271.9587600,-20.3157120,9.9859080,-0.0275110,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G9.9860-0.0276, 1,5(-1)->6(0)_A+,G10.322-0.148,G10.3563-0.1484,,15.0000000000,272.2629280,-20.0506890,10.3561720,-0.1485330,,,,49.82,,18.000,1.59 (0.03),2,1.65 (0.06),NGU22,1,,,NRAOVLA,+18 09 3.1028,-20 03 2.481,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,272.2629280,-20.0506890,10.3561720,-0.1485330,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G10.3562-0.1484, 1,5(-1)->6(0)_A+,G10.444-0.018,G10.4442-0.0182,,15.0000000000,272.1870420,-19.9106260,10.4441200,-0.0182670,,,,73.22,,18.000,26.35 (0.14),2,26.46 (0.25),NGU22,1,,,NRAOVLA,+18 08 44.89,-19 54 38.255,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,272.1870420,-19.9106260,10.4441200,-0.0182670,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G10.4442-0.0182, 1,5(-1)->6(0)_A+,G10.472+0.027,G10.4723+0.0273,,15.0000000000,272.1591850,-19.8638210,10.4723510,0.0273390,,,,74.92,,18.000,32.39 (0.12),2,32.85 (0.22),NGU22,1,,,NRAOVLA,+18 08 38.2044,-19 51 49.757,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,272.1591850,-19.8638210,10.4723510,0.0273390,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G10.4723+0.0264, 1,5(-1)->6(0)_A+,G10.472+0.027,G10.4800+0.0330,,15.0000000000,272.1578630,-19.8543640,10.4800180,0.0330140,,,,65.26,,18.000,13.62 (0.05),2,13.43 (0.1),NGU22,1,,,NRAOVLA,+18 08 37.887,-19 51 15.711,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,272.1578630,-19.8543640,10.4800180,0.0330140,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G10.4799+0.0330, 1,5(-1)->6(0)_A+,G10.623-0.383,G10.6266-0.3844,,15.0000000000,272.6218160,-19.9281110,10.6265500,-0.3844810,,,,4.42,,18.000,3.55 (0.03),2,3.54 (0.06),NGU22,1,,,NRAOVLA,+18 10 29.2358,-19 55 41.199,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,272.6218160,-19.9281110,10.6265500,-0.3844810,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G10.6235-0.3835, 1,5(-1)->6(0)_A+,G10.629-0.333,G10.6288-0.3330,,15.0000000000,272.5749500,-19.9012700,10.6287860,-0.3329350,,,,-0.4,,18.000,5.37 (0.08),2,5.23 (0.15),NGU22,1,,,NRAOVLA,+18 10 17.9881,-19 54 4.571,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,272.5749500,-19.9012700,10.6287860,-0.3329350,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G10.6287-0.3330, 1,5(-1)->6(0)_A+,G10.724-0.334,G10.7241-0.3343,,15.0000000000,272.6252110,-19.8185710,10.7240320,-0.3344140,,,,-2.28,,18.000,1.3 (0.03),2,1.3 (0.05),NGU22,1,,,NRAOVLA,+18 10 30.0506,-19 49 6.857,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,272.6252110,-19.8185710,10.7240320,-0.3344140,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G10.7240-0.3343, 1,5(-1)->6(0)_A+,G10.822-0.103,G10.8226-0.1030,,15.0000000000,272.4606600,-19.6204770,10.8226650,-0.1030970,,,,60.4,,18.000,0.49 (0.02),2,0.7 (0.05),NGU22,1,,,NRAOVLA,+18 09 50.5584,-19 37 13.716,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,272.4606600,-19.6204770,10.8226650,-0.1030970,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G10.8225-0.1030, 1,5(-1)->6(0)_A+,G10.885+0.123,G10.8857+0.1228,,15.0000000000,272.2831720,-19.4567050,10.8850430,0.1225320,,,,17.2,,18.000,5.99 (0.04),2,5.93 (0.07),NGU22,1,,,NRAOVLA,+18 09 7.9612,-19 27 24.139,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,272.2831720,-19.4567050,10.8850430,0.1225320,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G10.8851+0.1228, 1,5(-1)->6(0)_A+,G10.861+0.125,G10.8608+0.1248,,15.0000000000,272.2685120,-19.4769220,10.8606610,0.1248310,,,,20.08,,18.000,0.88 (0.02),2,1.03 (0.04),NGU22,1,,,NRAOVLA,+18 09 4.4428,-19 28 36.92,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,272.2685120,-19.4769220,10.8606610,0.1248310,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G10.8610+0.1254, 1,5(-1)->6(0)_A+,G10.958+0.022,G10.9584+0.0223,,15.0000000000,272.4137240,-19.4411210,10.9582640,0.0223540,,,,24.5,,18.000,17.63 (0.1),2,17.43 (0.17),NGU22,1,,,NRAOVLA,+18 09 39.2937,-19 26 28.037,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,272.4137240,-19.4411210,10.9582640,0.0223540,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G10.9583+0.0223, 1,5(-1)->6(0)_A+,G10.520+0.049,G10.5200+0.0492,,15.0000000000,272.1634620,-19.8115050,10.5200540,0.0491940,,,,38.4,,18.000,0.59 (0.02),2,0.67 (0.05),NGU22,1,,,NRAOVLA,+18 08 39.2308,-19 48 41.418,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,272.1634620,-19.8115050,10.5200540,0.0491940,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G10.5201+0.0492, 1,5(-1)->6(0)_A+,G10.635-0.407,G10.6353-0.4071,,15.0000000000,272.6468470,-19.9314090,10.6350160,-0.4066850,,,,-8.8,,18.000,0.75 (0.03),2,0.82 (0.06),NGU22,1,,,NRAOVLA,+18 10 35.2434,-19 55 53.074,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,272.6468470,-19.9314090,10.6350160,-0.4066850,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G10.6350-0.4067, 1,5(-1)->6(0)_A+,G10.205-0.345,G10.2049-0.3455,,15.0000000000,272.3684500,-20.2784460,10.2048500,-0.3454770,,,,6.66,,18.000,1.11 (0.04),2,1.11 (0.07),NGU22,1,,,NRAOVLA,+18 09 28.428,-20 16 42.407,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,272.3684500,-20.2784460,10.2048500,-0.3454770,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G10.2048-0.3455, 1,5(-1)->6(0)_A+,G10.322-0.148,G10.2873-0.1253,,15.0000000000,272.2057330,-20.0997340,10.2872380,-0.1253100,,,,3.42,,18.000,6.44 (0.05),2,6.86 (0.1),NGU22,1,,,NRAOVLA,+18 08 49.376,-20 05 59.041,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,272.2057330,-20.0997340,10.2872380,-0.1253100,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G10.2872-0.1252, 1,5(-1)->6(0)_A+,G10.322-0.148,G10.2994-0.1462,,15.0000000000,272.2314570,-20.0994540,10.2991920,-0.1463040,,,,10.28,,18.000,7.62 (0.18),2,8.04 (0.34),NGU22,1,,,NRAOVLA,+18 08 55.5497,-20 05 58.034,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,272.2314570,-20.0994540,10.2991920,-0.1463040,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G10.3013-0.1477, 1,5(-1)->6(0)_A+,G10.320-0.259,G10.3205-0.2586,,15.0000000000,272.3470820,-20.1352890,10.3204230,-0.2586470,,,,39,,18.000,9.53 (0.1),2,9.25 (0.18),NGU22,1,,,NRAOVLA,+18 09 23.2996,-20 08 7.04,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,272.3470820,-20.1352890,10.3204230,-0.2586470,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G10.3201-0.2586, 1,5(-1)->6(0)_A+,G10.320-0.259,G10.3069-0.2689,,15.0000000000,272.3501110,-20.1519790,10.3071940,-0.2692140,,,,26.76,,18.000,1.58 (0.03),2,1.53 (0.05),NGU22,1,,,NRAOVLA,+18 09 24.0267,-20 09 7.125,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,272.3501110,-20.1519790,10.3071940,-0.2692140,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G10.3072-0.2698, 1,5(-1)->6(0)_A+,G10.322-0.148,G10.3227-0.1598,,15.0000000000,272.2561790,-20.0855680,10.3225890,-0.1598850,,,,11.6,,18.000,73.41 (1.22),2,74.2 (2.23),NGU22,1,,,NRAOVLA,+18 09 1.483,-20 05 8.044,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,272.2561790,-20.0855680,10.3225890,-0.1598850,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G10.3226-0.1598, 1,5(-1)->6(0)_A+,G10.322-0.148,G10.3423-0.1423,,15.0000000000,272.2500460,-20.0598910,10.3422590,-0.1424050,,,,16.06,,18.000,15.04 (0.18),2,15.39 (0.33),NGU22,1,,,NRAOVLA,+18 09 0.0111,-20 03 35.609,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,272.2500460,-20.0598910,10.3422590,-0.1424050,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G10.3424-0.1423, 1,5(-1)->6(0)_A+,G10.373-0.185,G10.3735-0.1843,,15.0000000000,272.3052770,-20.0532180,10.3732280,-0.1845620,,,,16.78,,18.000,0.25 (0.03),2,0.58 (0.1),NGU22,1,,,NRAOVLA,+18 09 13.2665,-20 03 11.585,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,272.3052770,-20.0532180,10.3732280,-0.1845620,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G10.3732-0.1846, 1,5(-1)->6(0)_A+,G11.936-0.150,G11.9428-0.1560,,15.0000000000,273.0815040,-18.6645770,11.9428890,-0.1563630,,,,42.35,,18.000,5.31 (0.03),2,5.41 (0.06),NGU22,1,,,NRAOVLA,+18 12 19.5609,-18 39 52.476,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,273.0815040,-18.6645770,11.9428890,-0.1563630,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G11.9421-0.1552, 1,5(-1)->6(0)_A+,G11.904-0.141,G11.9041-0.1411,,15.0000000000,273.0476970,-18.6914340,11.9039470,-0.1411790,,,,43.21,,18.000,61.39 (0.13),2,61.37 (0.23),NGU22,1,,,NRAOVLA,+18 12 11.4473,-18 41 29.162,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,273.0476970,-18.6914340,11.9039470,-0.1411790,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G11.9040-0.1412, 1,5(-1)->6(0)_A+,G11.991-0.272,G11.9916-0.2723,,15.0000000000,273.2133160,-18.6778080,11.9912290,-0.2722600,,,,59.71,,18.000,2.28 (0.02),2,2.33 (0.04),NGU22,1,,,NRAOVLA,+18 12 51.1958,-18 40 40.11,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,273.2133160,-18.6778080,11.9912290,-0.2722600,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G11.9914-0.2722, 1,5(-1)->6(0)_A+,G11.111-0.400,G11.1110-0.3980,,15.0000000000,272.8823860,-19.5105330,11.1106600,-0.3981480,,,,5.31,,18.000,0.29 (0.02),2,0.33 (0.04),NGU22,1,,,NRAOVLA,+18 11 31.7726,-19 30 37.918,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,272.8823860,-19.5105330,11.1106600,-0.3981480,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G11.1105-0.3985, 1,5(-1)->6(0)_A+,G11.937-0.616,G11.9361-0.6156,,15.0000000000,273.5036920,-18.8906590,11.9360720,-0.6155360,,,,32.19,,18.000,34.87 (0.17),2,34.96 (0.29),NGU22,1,,,NRAOVLA,+18 14 0.886,-18 53 26.371,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,273.5036920,-18.8906590,11.9360720,-0.6155360,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G11.9365-0.6157, 1,5(-1)->6(0)_A+,G11.918-0.613,G11.9176-0.6132,,15.0000000000,273.4921940,-18.9045720,11.9186490,-0.6126380,,,,39.03,,18.000,3.98 (0.03),2,4.04 (0.06),NGU22,1,,,NRAOVLA,+18 13 58.1265,-18 54 16.458,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,273.4921940,-18.9045720,11.9186490,-0.6126380,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G11.9185-0.6126, 1,5(-1)->6(0)_A+,G11.034+0.062,G11.0339+0.0617,,15.0000000000,272.4160080,-19.3560320,11.0337800,0.0616250,,,,20.51,,18.000,0.38 (0.02),2,0.47 (0.04),NGU22,1,,,NRAOVLA,+18 09 39.8419,-19 21 21.715,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,272.4160080,-19.3560320,11.0337800,0.0616250,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G11.0339+0.0618, 1,5(-1)->6(0)_A+,G11.109-0.114,G11.1089-0.1140,,15.0000000000,272.6177280,-19.3751540,11.1089880,-0.1142340,,,,23.93,,18.000,21.93 (0.14),2,21.83 (0.24),NGU22,1,,,NRAOVLA,+18 10 28.2546,-19 22 30.556,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,272.6177280,-19.3751540,11.1089880,-0.1142340,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G11.1090-0.1140, 1,5(-1)->6(0)_A+,G11.903-0.102,G11.9034-0.1029,,15.0000000000,273.0112480,-18.6736380,11.9029570,-0.1023460,,,,33.73,,18.000,12.46 (0.05),2,12.46 (0.08),NGU22,1,,,NRAOVLA,+18 12 2.6994,-18 40 25.097,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,273.0112480,-18.6736380,11.9029570,-0.1023460,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G11.9031-0.1023, 1,5(-1)->6(0)_A+,G11.928-0.055,G11.9280-0.0550,,15.0000000000,272.9799390,-18.6288130,11.9279990,-0.0547840,,,,38.59,,18.000,0.55 (0.01),2,0.58 (0.02),NGU22,1,,,NRAOVLA,+18 11 55.1854,-18 37 43.728,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,272.9799390,-18.6288130,11.9279990,-0.0547840,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G11.9280-0.0548, 1,5(-1)->6(0)_A+,G11.841-0.101,G11.8397-0.1011,,15.0000000000,272.9778580,-18.7289000,11.8392960,-0.1011850,,,,21.49,,18.000,0.3 (0.03),2,0.54 (0.07),NGU22,1,,,NRAOVLA,+18 11 54.6859,-18 43 44.04,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,272.9778580,-18.7289000,11.8392960,-0.1011850,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G11.8393-0.1012, 1,5(-1)->6(0)_A+,G11.936-0.150,G11.9360-0.1501,,15.0000000000,273.0719950,-18.6675800,11.9359270,-0.1499040,,,,48.29,,18.000,2.17 (0.02),2,2.29 (0.04),NGU22,1,,,NRAOVLA,+18 12 17.2787,-18 40 3.288,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,273.0719950,-18.6675800,11.9359270,-0.1499040,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G11.9360-0.1499, 1,5(-1)->6(0)_A+,G12.627-0.017,G12.6248-0.0167,,15.0000000000,273.2970340,-17.9994700,12.6245920,-0.0166980,,,,21.78,,18.000,16.8 (0.03),2,16.94 (0.06),NGU22,1,,,NRAOVLA,+18 13 11.2881,-17 59 58.092,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,273.2970340,-17.9994700,12.6245920,-0.0166980,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G12.6247-0.0167, 1,5(-1)->6(0)_A+,G12.681-0.182,G12.6807-0.1823,,15.0000000000,273.4780780,-18.0296340,12.6805690,-0.1822840,,,,58.4,,18.000,942.93 (3.57),2,960.42 (6.52),NGU22,1,,,NRAOVLA,+18 13 54.7387,-18 01 46.681,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,273.4780780,-18.0296340,12.6805690,-0.1822840,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G12.6806-0.1823, 1,5(-1)->6(0)_A+,G12.889+0.490,G12.8888+0.4892,,15.0000000000,272.9638520,-17.5252810,12.8882080,0.4893070,,,,39.2,,18.000,56.84 (0.76),2,58.42 (1.38),NGU22,1,,,NRAOVLA,+18 11 51.3245,-17 31 31.012,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,272.9638520,-17.5252810,12.8882080,0.4893070,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G12.8887+0.4898, 1,5(-1)->6(0)_A+,G12.904-0.031,G12.9044-0.0311,,15.0000000000,273.4510680,-17.7609540,12.9041830,-0.0311340,,,,59.28,,18.000,32.1 (0.18),2,32.13 (0.32),NGU22,1,,,NRAOVLA,+18 13 48.2563,-17 45 39.435,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,273.4510680,-17.7609540,12.9041830,-0.0311340,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G12.9044-0.0310, 1,5(-1)->6(0)_A+,G12.908-0.260,G12.9087-0.2603,,15.0000000000,273.6645100,-17.8663000,12.9088200,-0.2599790,,,,39.18,,18.000,225.62 (1.76),2,233.33 (3.28),NGU22,1,,,NRAOVLA,+18 14 39.4823,-17 51 58.681,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,273.6645100,-17.8663000,12.9088200,-0.2599790,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G12.9085-0.2602, 1,5(-1)->6(0)_A+,G12.418+0.504,G12.4193+0.5027,,15.0000000000,272.7142050,-17.9303420,12.4186800,0.5026800,,,,23.16,,18.000,2.49 (0.03),2,2.56 (0.06),NGU22,1,,,NRAOVLA,+18 10 51.4091,-17 55 49.23,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,272.7142050,-17.9303420,12.4186800,0.5026800,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G12.4179+0.5037, 1,5(-1)->6(0)_A+,G12.120-0.270,G12.1206-0.2703,,15.0000000000,273.2768280,-18.5638410,12.1201010,-0.2704170,,,,0.28,,18.000,0.47 (0.02),2,0.53 (0.03),NGU22,1,,,NRAOVLA,+18 13 6.4386,-18 33 49.828,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,273.2768280,-18.5638410,12.1201010,-0.2704170,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G12.1201-0.2704, 1,5(-1)->6(0)_A+,G12.082-0.506,G12.0824-0.5064,,15.0000000000,273.4760910,-18.7100400,12.0821910,-0.5061880,,,,32.24,,18.000,0.43 (0.03),2,0.41 (0.05),NGU22,1,,,NRAOVLA,+18 13 54.2619,-18 42 36.145,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,273.4760910,-18.7100400,12.0821910,-0.5061880,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G12.0822-0.5062, 1,5(-1)->6(0)_A+,G12.025-0.032,G12.0255-0.0314,,15.0000000000,273.0076650,-18.5323050,12.0252560,-0.0314260,,,,108.12,,18.000,99.7 (0.48),2,98.85 (0.85),NGU22,1,,,NRAOVLA,+18 12 1.8396,-18 31 56.298,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,273.0076650,-18.5323050,12.0252560,-0.0314260,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G12.0254-0.0315, 1,5(-1)->6(0)_A+,G12.112-0.126,G12.1117-0.1263,,15.0000000000,273.1390680,-18.5022190,12.1115030,-0.1262520,,,,39.54,,18.000,2.07 (0.01),2,2.04 (0.03),NGU22,1,,,NRAOVLA,+18 12 33.3764,-18 30 7.988,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,273.1390680,-18.5022190,12.1115030,-0.1262520,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G12.1116-0.1262, 1,5(-1)->6(0)_A+,G12.209-0.107,G12.1811-0.1225,,15.0000000000,273.1708380,-18.4393070,12.1811580,-0.1224870,,,,29.52,,18.000,1.63 (0.02),2,1.63 (0.03),NGU22,1,,,NRAOVLA,+18 12 41.0012,-18 26 21.504,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,273.1708380,-18.4393070,12.1811580,-0.1224870,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G12.1811-0.1225, 1,5(-1)->6(0)_A+,G12.199-0.034,G12.1993-0.0335,,15.0000000000,273.0976250,-18.3807660,12.1991580,-0.0334440,,,,49.3,,18.000,10.54 (0.05),2,10.55 (0.1),NGU22,1,,,NRAOVLA,+18 12 23.4301,-18 22 50.757,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,273.0976250,-18.3807660,12.1991580,-0.0334440,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G12.1991-0.0336, 1,5(-1)->6(0)_A+,G12.209-0.107,G12.2019-0.1199,,15.0000000000,273.1787320,-18.4193580,12.2022530,-0.1194830,,,,29.64,,18.000,0.27 (0.02),2,0.26 (0.03),NGU22,1,,,NRAOVLA,+18 12 42.8956,-18 25 9.69,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,273.1787320,-18.4193580,12.2022530,-0.1194830,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G12.2020-0.1198, 1,5(-1)->6(0)_A+,G12.209-0.107,G12.2027-0.1073,,15.0000000000,273.1676220,-18.4130160,12.2027590,-0.1071910,,,,17.26,,18.000,2.15 (0.17),2,2.63 (0.35),NGU22,1,,,NRAOVLA,+18 12 40.2293,-18 24 46.856,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,273.1676220,-18.4130160,12.2027590,-0.1071910,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G12.2026-0.1072, 1,5(-1)->6(0)_A+,G12.209-0.107,G12.2093-0.1023,,15.0000000000,273.1662900,-18.4050350,12.2091540,-0.1022520,,,,19.8,,18.000,9.4 (0.07),2,9.55 (0.13),NGU22,1,,,NRAOVLA,+18 12 39.9097,-18 24 18.125,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,273.1662900,-18.4050350,12.2091540,-0.1022520,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G12.2092-0.1023, 1,5(-1)->6(0)_A+,G12.265-0.051,G12.2654-0.0512,,15.0000000000,273.1475170,-18.3311670,12.2654020,-0.0511640,,,,68.48,,18.000,3.41 (0.02),2,3.38 (0.04),NGU22,1,,,NRAOVLA,+18 12 35.404,-18 19 52.202,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,273.1475170,-18.3311670,12.2654020,-0.0511640,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G12.2654-0.0512, 1,5(-1)->6(0)_A+,G12.526+0.016,G12.5258+0.0162,,15.0000000000,273.2168060,-18.0706780,12.5255230,0.0160960,,,,42.5,,18.000,6.68 (0.06),2,6.81 (0.1),NGU22,1,,,NRAOVLA,+18 12 52.0335,-18 04 14.442,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,273.2168060,-18.0706780,12.5255230,0.0160960,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G12.5257+0.0162, 1,5(-1)->6(0)_A+,G13.179+0.060,G13.1793+0.0612,,15.0000000000,273.5039940,-17.4756860,13.1788100,0.0610750,,,,46.54,,18.000,2.31 (0.02),2,2.35 (0.04),NGU22,1,,,NRAOVLA,+18 14 0.9585,-17 28 32.471,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,273.5039940,-17.4756860,13.1788100,0.0610750,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G13.1789+0.0603, 1,5(-1)->6(0)_A+,G13.657-0.600,G13.6570-0.5992,,15.0000000000,274.3510400,-17.3702990,13.6565320,-0.5992700,,,,51.04,,18.000,32.14 (0.18),2,32.59 (0.33),NGU22,1,,,NRAOVLA,+18 17 24.2496,-17 22 13.075,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,274.3510400,-17.3702990,13.6565320,-0.5992700,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G13.6567-0.5998, 1,5(-1)->6(0)_A+,G13.696-0.156,G13.6966-0.1562,,15.0000000000,273.9627670,-17.1248090,13.6962150,-0.1563340,,,,99.23,,18.000,1.91 (0.02),2,1.99 (0.03),NGU22,1,,,NRAOVLA,+18 15 51.0641,-17 07 29.313,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,273.9627670,-17.1248090,13.6962150,-0.1563340,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G13.6961-0.1563, 1,5(-1)->6(0)_A+,G13.713-0.084,G13.7126-0.0839,,15.0000000000,273.9040390,-17.0756050,13.7127330,-0.0835400,,,,43.43,,18.000,32 (0.22),2,31.87 (0.38),NGU22,1,,,NRAOVLA,+18 15 36.9694,-17 04 32.178,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,273.9040390,-17.0756050,13.7127330,-0.0835400,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G13.7129-0.0836, 1,5(-1)->6(0)_A+,G14.606+0.016,G14.6072+0.0089,,15.0000000000,274.2634210,-16.2448180,14.6072710,0.0088970,,,,27.3,,18.000,0.41 (0.02),2,0.47 (0.04),NGU22,1,,,NRAOVLA,+18 17 3.2211,-16 14 41.346,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,274.2634210,-16.2448180,14.6072710,0.0088970,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G14.6060+0.0129, 1,5(-1)->6(0)_A+,G14.606+0.016,G14.5849+0.0176,,15.0000000000,274.2435430,-16.2616120,14.5834280,0.0177120,,,,25.5,,18.000,0.4 (0.02),2,0.36 (0.03),NGU22,1,,,NRAOVLA,+18 16 58.4504,-16 15 41.803,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,274.2435430,-16.2616120,14.5834280,0.0177120,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G14.5834+0.0177, 1,5(-1)->6(0)_A+,G14.521+0.155,G14.5204+0.1547,,15.0000000000,274.0863920,-16.2516340,14.5204820,0.1551840,,,,2.93,,18.000,0.57 (0.02),2,0.62 (0.03),NGU22,1,,,NRAOVLA,+18 16 20.7341,-16 15 5.882,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,274.0863920,-16.2516340,14.5204820,0.1551840,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G14.5206+0.1552, 1,5(-1)->6(0)_A+,G14.519+0.116,G14.5202+0.1161,,15.0000000000,274.1220770,-16.2714130,14.5193800,0.1156420,,,,14.99,,18.000,0.13 (0.02),2,0.23 (0.04),NGU22,1,,,NRAOVLA,+18 16 29.2986,-16 16 17.085,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,274.1220770,-16.2714130,14.5193800,0.1156420,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G14.5194+0.1156, 1,5(-1)->6(0)_A+,G14.631-0.577,G14.6315-0.5772,,15.0000000000,274.8132820,-16.5011640,14.6314870,-0.5771470,,,,25.05,,18.000,3.03 (0.02),2,2.99 (0.03),NGU22,1,,,NRAOVLA,+18 19 15.1876,-16 30 4.191,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,274.8132820,-16.5011640,14.6314870,-0.5771470,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G14.6314-0.5772, 1,5(-1)->6(0)_A+,G14.991-0.121,G14.9905-0.1217,,15.0000000000,274.5721570,-15.9688290,14.9909320,-0.1213170,,,,46.09,,18.000,5.77 (0.08),2,5.97 (0.14),NGU22,1,,,NRAOVLA,+18 18 17.3176,-15 58 7.784,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,274.5721570,-15.9688290,14.9909320,-0.1213170,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G14.9908-0.1214, 1,5(-1)->6(0)_A+,G14.101+0.087,G14.1015+0.0870,,15.0000000000,273.9409560,-16.6526960,14.1013810,0.0869080,,,,15.04,,18.000,89.2 (0.23),2,89.22 (0.41),NGU22,1,,,NRAOVLA,+18 15 45.8294,-16 39 9.706,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,273.9409560,-16.6526960,14.1013810,0.0869080,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G14.1014+0.0870, 1,5(-1)->6(0)_A+,G14.230-0.509,G14.2298-0.5093,,15.0000000000,274.5524170,-16.8226390,14.2300090,-0.5090870,,,,25.3,,18.000,0.22 (0.02),2,0.23 (0.04),NGU22,1,,,NRAOVLA,+18 18 12.5801,-16 49 21.5,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,274.5524170,-16.8226390,14.2300090,-0.5090870,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G14.2297-0.5093, 1,5(-1)->6(0)_A+,G14.332-0.642,G14.3311-0.6414,,15.0000000000,274.7264600,-16.7973960,14.3311090,-0.6439010,,,,21.56,,18.000,0.55 (0.02),2,0.54 (0.04),NGU22,1,,,NRAOVLA,+18 18 54.3505,-16 47 50.627,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,274.7264600,-16.7973960,14.3311090,-0.6439010,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G14.3317-0.6419, 1,5(-1)->6(0)_A+,G14.390-0.020,G14.3896-0.0203,,15.0000000000,274.1823450,-16.4504540,14.3893660,-0.0203600,,,,27.26,,18.000,1.9 (0.02),2,1.87 (0.04),NGU22,1,,,NRAOVLA,+18 16 43.7628,-16 27 1.635,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,274.1823450,-16.4504540,14.3893660,-0.0203600,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G14.3895-0.0203, 1,5(-1)->6(0)_A+,G14.444-0.063,G14.4417-0.0640,,15.0000000000,274.2483060,-16.4248120,14.4419910,-0.0638400,,,,28.16,,18.000,0.16 (0.02),2,0.28 (0.05),NGU22,1,,,NRAOVLA,+18 16 59.5934,-16 25 29.323,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,274.2483060,-16.4248120,14.4419910,-0.0638400,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G14.4428-0.0635, 1,5(-1)->6(0)_A+,G14.442-0.151,G14.4567-0.1434,,15.0000000000,274.3282010,-16.4494710,14.4566800,-0.1429890,,,,38.24,,18.000,1.31 (0.03),2,1.42 (0.06),NGU22,1,,,NRAOVLA,+18 17 18.7683,-16 26 58.097,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,274.3282010,-16.4494710,14.4566800,-0.1429890,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G14.4568-0.1430, 1,5(-1)->6(0)_A+,G14.490+0.014,G14.4897+0.0142,,15.0000000000,274.2001530,-16.3464010,14.4890350,0.0140670,,,,20.2,,18.000,1.2 (0.01),2,1.25 (0.02),NGU22,1,,,NRAOVLA,+18 16 48.0368,-16 20 47.042,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,274.2001530,-16.3464010,14.4890350,0.0140670,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G14.4896+0.0141, 1,5(-1)->6(0)_A+,G14.767+0.286,G14.7669+0.2853,,15.0000000000,274.0887510,-15.9730260,14.7666210,0.2857360,,,,23.3,,18.000,1.49 (0.02),2,1.52 (0.03),NGU22,1,,,NRAOVLA,+18 16 21.3002,-15 58 22.893,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,274.0887510,-15.9730260,14.7666210,0.2857360,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G14.7666+0.2857, 1,5(-1)->6(0)_A+,G14.606+0.016,G14.6037+0.0165,,15.0000000000,274.2547790,-16.2441960,14.6038770,0.0164940,,,,34.68,,18.000,3.15 (0.02),2,3.19 (0.04),NGU22,1,,,NRAOVLA,+18 17 1.1469,-16 14 39.107,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,274.2547790,-16.2441960,14.6038770,0.0164940,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G14.6060+0.0129, 1,5(-1)->6(0)_A+,G15.029+0.852,G15.0319+0.8501,,15.0000000000,273.7041460,-15.4717350,15.0309400,0.8500890,,,,49.48,,18.000,0.36 (0.02),2,0.47 (0.04),NGU22,1,,,NRAOVLA,+18 14 48.9951,-15 28 18.246,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,273.7041460,-15.4717350,15.0309400,0.8500890,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G15.0294+0.8520, 1,5(-1)->6(0)_A+,G15.094+0.191,G15.0943+0.1913,,15.0000000000,274.3368980,-15.7292530,15.0945500,0.1915390,,,,25.72,,18.000,14.18 (0.31),2,15.5 (0.61),NGU22,1,,,NRAOVLA,+18 17 20.8556,-15 43 45.31,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,274.3368980,-15.7292530,15.0945500,0.1915390,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G15.0942+0.1915, 1,5(-1)->6(0)_A+,G15.665-0.499,G15.6658-0.4989,,15.0000000000,275.2490240,-15.5526740,15.6654160,-0.4989640,,,,-3.09,,18.000,22.53 (0.33),2,24.04 (0.63),NGU22,1,,,NRAOVLA,+18 20 59.7658,-15 33 9.627,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,275.2490240,-15.5526740,15.6654160,-0.4989640,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G15.6651-0.4990, 1,5(-1)->6(0)_A+,G15.607-0.255,G15.6061-0.2559,,15.0000000000,274.9972620,-15.4899640,15.6063600,-0.2554680,,,,66.05,,18.000,0.73 (0.02),2,0.77 (0.04),NGU22,1,,,NRAOVLA,+18 19 59.3429,-15 29 23.872,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,274.9972620,-15.4899640,15.6063600,-0.2554680,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G15.6066-0.2553, 1,5(-1)->6(0)_A+,G15.557-0.464,G15.5589-0.4642,,15.0000000000,275.1651740,-15.6305500,15.5586720,-0.4644080,,,,17.27,,18.000,0.51 (0.02),2,0.66 (0.04),NGU22,1,,,NRAOVLA,+18 20 39.6418,-15 37 49.98,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,275.1651740,-15.6305500,15.5586720,-0.4644080,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G15.5566-0.4635, 1,5(-1)->6(0)_A+,G15.271-0.120,G15.2707-0.1198,,15.0000000000,274.7084670,-15.7222310,15.2702250,-0.1200830,,,,32.56,,18.000,2.03 (0.03),2,2.17 (0.07),NGU22,1,,,NRAOVLA,+18 18 50.032,-15 43 20.032,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,274.7084670,-15.7222310,15.2702250,-0.1200830,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G15.2707-0.1207, 1,5(-1)->6(0)_A+,G15.033-0.674,G15.0345-0.6774,,15.0000000000,275.1033870,-16.1932040,15.0344040,-0.6772010,,,,21.23,,18.000,37.31 (0.36),2,39.58 (0.69),NGU22,1,,,NRAOVLA,+18 20 24.813,-16 11 35.534,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,275.1033870,-16.1932040,15.0344040,-0.6772010,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G15.0345-0.6770, 1,5(-1)->6(0)_A+,G16.976-0.005,G16.9764-0.0047,,15.0000000000,275.4360150,-14.1634150,16.9762980,-0.0046600,,,,6.8,,18.000,0.32 (0.02),2,0.37 (0.05),NGU22,1,,,NRAOVLA,+18 21 44.6436,-14 09 48.294,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,275.4360150,-14.1634150,16.9762980,-0.0046600,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G16.9763-0.0048, 1,5(-1)->6(0)_A+,G16.651-0.305,G16.6514-0.3047,,15.0000000000,275.5515360,-14.5914070,16.6511280,-0.3046020,,,,33.64,,18.000,0.6 (0.02),2,0.71 (0.03),NGU22,1,,,NRAOVLA,+18 22 12.3686,-14 35 29.064,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,275.5515360,-14.5914070,16.6511280,-0.3046020,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G16.6511-0.3046, 1,5(-1)->6(0)_A+,G16.610-0.236,G16.6091-0.2380,,15.0000000000,275.4701130,-14.5973520,16.6088490,-0.2378440,,,,44.97,,18.000,0.43 (0.02),2,0.48 (0.05),NGU22,1,,,NRAOVLA,+18 21 52.8272,-14 35 50.468,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,275.4701130,-14.5973520,16.6088490,-0.2378440,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G16.6097-0.2365, 1,5(-1)->6(0)_A+,G16.403-0.181,G16.4029-0.1812,,15.0000000000,275.3185470,-14.7522680,16.4031700,-0.1813310,,,,39.2,,18.000,0.24 (0.02),2,0.27 (0.04),NGU22,1,,,NRAOVLA,+18 21 16.4513,-14 45 8.166,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,275.3185470,-14.7522680,16.4031700,-0.1813310,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G16.4029-0.1812, 1,5(-1)->6(0)_A+,G16.855+0.641,G16.8550+0.6412,,15.0000000000,274.7898910,-13.9660730,16.8548290,0.6411030,,,,24.2,,18.000,1.16 (0.03),2,1.23 (0.06),NGU22,1,,,NRAOVLA,+18 19 9.5738,-13 57 57.863,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,274.7898910,-13.9660730,16.8548290,0.6411030,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G16.8549+0.6411, 1,5(-1)->6(0)_A+,G16.117-0.291,G16.1111-0.3054,,15.0000000000,275.2881080,-15.0668050,16.1118150,-0.3034470,,,,34.54,,18.000,1.47 (0.03),2,1.61 (0.06),NGU22,1,,,NRAOVLA,+18 21 9.1458,-15 04 0.498,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,275.2881080,-15.0668050,16.1118150,-0.3034470,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G16.1118-0.3034, 1,5(-1)->6(0)_A+,G16.302-0.196,G16.3014-0.1963,,15.0000000000,275.2827060,-14.8486930,16.3017850,-0.1961530,,,,51.8,,18.000,9.95 (0.15),2,10.85 (0.29),NGU22,1,,,NRAOVLA,+18 21 7.8495,-14 50 55.296,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,275.2827060,-14.8486930,16.3017850,-0.1961530,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G16.3019-0.1960, 1,5(-1)->6(0)_A+,G16.302-0.196,G16.3079-0.2037,,15.0000000000,275.2924440,-14.8471520,16.3075770,-0.2037310,,,,41,,18.000,0.35 (0.02),2,0.35 (0.04),NGU22,1,,,NRAOVLA,+18 21 10.1866,-14 50 49.746,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,275.2924440,-14.8471520,16.3075770,-0.2037310,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G16.3076-0.2037, 1,5(-1)->6(0)_A+,G16.337-0.224,G16.3372-0.2236,,15.0000000000,275.3249700,-14.8303770,16.3371770,-0.2235750,,,,45.68,,18.000,0.39 (0.02),2,0.41 (0.03),NGU22,1,,,NRAOVLA,+18 21 17.9928,-14 49 49.358,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,275.3249700,-14.8303770,16.3371770,-0.2235750,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G16.3372-0.2236, 1,5(-1)->6(0)_A+,G16.585-0.051,G16.5855-0.0505,,15.0000000000,275.2880110,-14.5301620,16.5852190,-0.0507060,,,,62.09,,18.000,51.65 (0.55),2,54.27 (1.02),NGU22,1,,,NRAOVLA,+18 21 9.1227,-14 31 48.582,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,275.2880110,-14.5301620,16.5852190,-0.0507060,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G16.5852-0.0507, 1,5(-1)->6(0)_A+,G16.662-0.331,G16.6612-0.3318,,15.0000000000,275.5809780,-14.5947770,16.6615370,-0.3313380,,,,42.99,,18.000,3.39 (0.03),2,3.53 (0.06),NGU22,1,,,NRAOVLA,+18 22 19.4348,-14 35 41.198,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,275.5809780,-14.5947770,16.6615370,-0.3313380,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G16.6621-0.3312, 1,5(-1)->6(0)_A+,G16.831+0.079,G16.8313+0.0787,,15.0000000000,275.2896820,-14.2526890,16.8307750,0.0785050,,,,58.68,,18.000,5.08 (0.05),2,5.32 (0.09),NGU22,1,,,NRAOVLA,+18 21 9.5237,-14 15 9.681,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,275.2896820,-14.2526890,16.8307750,0.0785050,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G16.8311+0.0786, 1,5(-1)->6(0)_A+,G17.029-0.071,G17.0298-0.0707,,15.0000000000,275.5216970,-14.1470470,17.0298000,-0.0702940,,,,91.23,,18.000,0.74 (0.02),2,0.9 (0.05),NGU22,1,,,NRAOVLA,+18 22 5.2072,-14 08 49.371,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,275.5216970,-14.1470470,17.0298000,-0.0702940,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G17.0294-0.0705, 1,5(-1)->6(0)_A+,G17.638+0.157,G17.6396+0.1564,,15.0000000000,275.6097580,-13.5035750,17.6380200,0.1565060,,,,20.69,,18.000,20.52 (0.27),2,21.89 (0.5),NGU22,1,,,NRAOVLA,+18 22 26.3418,-13 30 12.87,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,275.6097580,-13.5035750,17.6380200,0.1565060,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G17.6383+0.1565, 1,5(-1)->6(0)_A+,G17.862+0.074,G17.8618+0.0745,,15.0000000000,275.7919500,-13.3444230,17.8617220,0.0747020,,,,108.17,,18.000,1.22 (0.02),2,1.4 (0.04),NGU22,1,,,NRAOVLA,+18 23 10.068,-13 20 39.924,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,275.7919500,-13.3444230,17.8617220,0.0747020,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G17.8616+0.0745, 1,5(-1)->6(0)_A+,G17.035+0.748,G17.0346+0.7488,,15.0000000000,274.7796210,-13.7569130,17.0344470,0.7487570,,,,20.87,,18.000,0.31 (0.02),2,0.32 (0.03),NGU22,1,,,NRAOVLA,+18 19 7.109,-13 45 24.887,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,274.7796210,-13.7569130,17.0344470,0.7487570,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G17.0351+0.7481, 1,5(-1)->6(0)_A+,G17.595+0.089,G17.5944+0.0856,,15.0000000000,275.6528540,-13.5753960,17.5942800,0.0857910,,,,24.83,,18.000,0.51 (0.02),2,0.62 (0.04),NGU22,1,,,NRAOVLA,+18 22 36.685,-13 34 31.426,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,275.6528540,-13.5753960,17.5942800,0.0857910,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G17.5943+0.0858, 1,5(-1)->6(0)_A+,G18.834-0.300,G18.8341-0.3003,,15.0000000000,276.5982860,-12.6605270,18.8335970,-0.3000460,,,,41.19,,18.000,4.48 (0.05),2,4.34 (0.09),NGU22,1,,,NRAOVLA,+18 26 23.5887,-12 39 37.897,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.5982860,-12.6605270,18.8335970,-0.3000460,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G18.8337-0.3003, 1,5(-1)->6(0)_A+,G18.874+0.053,G18.8737+0.0532,,15.0000000000,276.2973140,-12.4605600,18.8733550,0.0530920,,,,38.49,,18.000,10.6 (0.24),2,10.72 (0.43),NGU22,1,,,NRAOVLA,+18 25 11.3553,-12 27 38.016,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.2973140,-12.4605600,18.8733550,0.0530920,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G18.8736+0.0533, 1,5(-1)->6(0)_A+,G18.888-0.475,G18.8883-0.4746,,15.0000000000,276.7827220,-12.6934730,18.8882740,-0.4746150,,,,54.9,,18.000,2.06 (0.04),2,2.23 (0.07),NGU22,1,,,NRAOVLA,+18 27 7.8534,-12 41 36.504,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.7827220,-12.6934730,18.8882740,-0.4746150,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G18.8884-0.4747, 1,5(-1)->6(0)_A+,G18.073+0.077,G18.0730+0.0768,,15.0000000000,275.8916740,-13.1572570,18.0725530,0.0766970,,,,55.62,,18.000,5.29 (0.11),2,5.47 (0.2),NGU22,1,,,NRAOVLA,+18 23 34.0017,-13 09 26.124,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,275.8916740,-13.1572570,18.0725530,0.0766970,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G18.0728+0.0769, 1,5(-1)->6(0)_A+,G18.159+0.094,G18.1599+0.0942,,15.0000000000,275.9175510,-13.0722730,18.1594400,0.0942510,,,,58.32,,18.000,7.33 (0.11),2,7.5 (0.19),NGU22,1,,,NRAOVLA,+18 23 40.2123,-13 04 20.182,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,275.9175510,-13.0722730,18.1594400,0.0942510,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G18.1592+0.0943, 1,5(-1)->6(0)_A+,G18.262-0.244,G18.2647-0.2440,,15.0000000000,276.2735580,-13.1398940,18.2619050,-0.2438280,,,,75.76,,18.000,17.95 (0.29),2,19.21 (0.55),NGU22,1,,,NRAOVLA,+18 25 5.6539,-13 08 23.617,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.2735580,-13.1398940,18.2619050,-0.2438280,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G18.2621-0.2439, 1,5(-1)->6(0)_A+,G18.440+0.045,G18.4397+0.0442,,15.0000000000,276.0971070,-12.8482170,18.4393460,0.0445300,,,,62.09,,18.000,2 (0.05),2,1.89 (0.08),NGU22,1,,,NRAOVLA,+18 24 23.3058,-12 50 53.582,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.0971070,-12.8482170,18.4393460,0.0445300,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G18.4397+0.0447, 1,5(-1)->6(0)_A+,G18.461-0.004,G18.4605-0.0044,,15.0000000000,276.1513610,-12.8524230,18.4603720,-0.0041880,,,,49.46,,18.000,19.33 (0.17),2,19.57 (0.3),NGU22,1,,,NRAOVLA,+18 24 36.3267,-12 51 8.723,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.1513610,-12.8524230,18.4603720,-0.0041880,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G18.4606-0.0042, 1,5(-1)->6(0)_A+,G18.666+0.032,G18.6619+0.0345,,15.0000000000,276.2126800,-12.6566750,18.6613680,0.0344740,,,,80.25,,18.000,5.68 (0.08),2,5.74 (0.15),NGU22,1,,,NRAOVLA,+18 24 51.0432,-12 39 24.029,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.2126800,-12.6566750,18.6613680,0.0344740,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G18.6618+0.0346, 1,5(-1)->6(0)_A+,G18.666+0.032,G18.6667+0.0247,,15.0000000000,276.2237880,-12.6564110,18.6666670,0.0250160,,,,78.64,,18.000,12.6 (0.16),2,12.86 (0.29),NGU22,1,,,NRAOVLA,+18 24 53.7091,-12 39 23.081,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.2237880,-12.6564110,18.6666670,0.0250160,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G18.6674+0.0251, 1,5(-1)->6(0)_A+,G18.735-0.225,G18.7341-0.2239,,15.0000000000,276.4814620,-12.7133090,18.7337520,-0.2238440,,,,45.86,,18.000,1.32 (0.03),2,1.4 (0.06),NGU22,1,,,NRAOVLA,+18 25 55.5509,-12 42 47.912,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.4814620,-12.7133090,18.7337520,-0.2238440,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G18.7350-0.2255, 1,5(-1)->6(0)_A+,G18.735-0.225,G18.7355-0.2273,,15.0000000000,276.4853110,-12.7137030,18.7351550,-0.2273490,,,,38.13,,18.000,1.88 (0.04),2,1.85 (0.07),NGU22,1,,,NRAOVLA,+18 25 56.4747,-12 42 49.331,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.4853110,-12.7137030,18.7351550,-0.2273490,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G18.7350-0.2255, 1,5(-1)->6(0)_A+,G19.485+0.151,G19.4868+0.1508,,15.0000000000,276.5015670,-11.8727920,19.4863550,0.1509190,,,,19.96,,18.000,5.03 (0.1),2,5.44 (0.19),NGU22,1,,,NRAOVLA,+18 26 0.376,-11 52 22.05,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.5015670,-11.8727920,19.4863550,0.1509190,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G19.4862+0.1508, 1,5(-1)->6(0)_A+,G19.609-0.234,G19.6084-0.2346,,15.0000000000,276.9079330,-11.9441040,19.6084890,-0.2341400,,,,41.55,,18.000,0.22 (0.02),2,0.25 (0.04),NGU22,1,,,NRAOVLA,+18 27 37.9038,-11 56 38.775,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.9079330,-11.9441040,19.6084890,-0.2341400,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G19.6090-0.2344, 1,5(-1)->6(0)_A+,G19.640-0.176,G19.6370-0.1835,,15.0000000000,276.8759010,-11.8952540,19.6371480,-0.1836700,,,,38.49,,18.000,0.25 (0.02),2,0.28 (0.04),NGU22,1,,,NRAOVLA,+18 27 30.2163,-11 53 42.915,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.8759010,-11.8952540,19.6371480,-0.1836700,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G19.6371-0.1837, 1,5(-1)->6(0)_A+,G19.612-0.134,G19.6118-0.1200,,15.0000000000,276.8061290,-11.8894480,19.6105100,-0.1205390,,,,57.74,,18.000,1.3 (0.03),2,1.44 (0.06),NGU22,1,,,NRAOVLA,+18 27 13.471,-11 53 22.014,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.8061290,-11.8894480,19.6105100,-0.1205390,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G19.6121-0.1199, 1,5(-1)->6(0)_A+,G19.612-0.134,G19.6125-0.1339,,15.0000000000,276.8186500,-11.8941340,19.6120660,-0.1335640,,,,56.52,,18.000,11.25 (0.16),2,12.03 (0.3),NGU22,1,,,NRAOVLA,+18 27 16.476,-11 53 38.884,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.8186500,-11.8941340,19.6120660,-0.1335640,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G19.6122-0.1337, 1,5(-1)->6(0)_A+,G19.614+0.011,G19.6139+0.0112,,15.0000000000,276.6883360,-11.8256880,19.6132450,0.0111700,,,,31.84,,18.000,2.96 (0.02),2,3.17 (0.04),NGU22,1,,,NRAOVLA,+18 26 45.2007,-11 49 32.476,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.6883360,-11.8256880,19.6132450,0.0111700,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G19.6136+0.0112, 1,5(-1)->6(0)_A+,G19.667+0.114,G19.6667+0.1140,,15.0000000000,276.6205630,-11.7303760,19.6666560,0.1142890,,,,16.19,,18.000,1.57 (0.02),2,1.67 (0.03),NGU22,1,,,NRAOVLA,+18 26 28.9351,-11 43 49.353,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.6205630,-11.7303760,19.6666560,0.1142890,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G19.6668+0.1142, 1,5(-1)->6(0)_A+,G19.701-0.267,G19.7007-0.2672,,15.0000000000,276.9810660,-11.8781870,19.7001260,-0.2668300,,,,43.71,,18.000,8.38 (0.12),2,8.88 (0.23),NGU22,1,,,NRAOVLA,+18 27 55.4559,-11 52 41.472,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.9810660,-11.8781870,19.7001260,-0.2668300,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G19.7005-0.2668, 1,5(-1)->6(0)_A+,G19.754-0.128,G19.7549-0.1284,,15.0000000000,276.8816710,-11.7651860,19.7549060,-0.1281470,,,,116.27,,18.000,1.56 (0.02),2,1.69 (0.05),NGU22,1,,,NRAOVLA,+18 27 31.6011,-11 45 54.67,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.8816710,-11.7651860,19.7549060,-0.1281470,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G19.7547-0.1281, 1,5(-1)->6(0)_A+,G19.009-0.029,G19.0084-0.0284,,15.0000000000,276.4363850,-12.3796650,19.0083090,-0.0292330,,,,54.72,,18.000,23.65 (0.18),2,25.01 (0.33),NGU22,1,,,NRAOVLA,+18 25 44.7323,-12 22 46.795,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.4363850,-12.3796650,19.0083090,-0.0292330,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G19.0086-0.0293, 1,5(-1)->6(0)_A+,G19.249+0.267,G19.2486+0.2668,,15.0000000000,276.2832570,-12.0287250,19.2487460,0.2669930,,,,19.79,,18.000,1.69 (0.04),2,1.87 (0.08),NGU22,1,,,NRAOVLA,+18 25 7.9818,-12 01 43.409,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.2832570,-12.0287250,19.2487460,0.2669930,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G19.2491+0.2670, 1,5(-1)->6(0)_A+,G19.267+0.349,G19.2668+0.3487,,15.0000000000,276.2181370,-11.9745270,19.2668940,0.3486340,,,,16.19,,18.000,4.35 (0.12),2,4.7 (0.23),NGU22,1,,,NRAOVLA,+18 24 52.3529,-11 58 28.297,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.2181370,-11.9745270,19.2668940,0.3486340,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G19.2670+0.3485, 1,5(-1)->6(0)_A+,G19.278+0.305,G19.2766+0.3041,,15.0000000000,276.2626070,-11.9869280,19.2762620,0.3043810,,,,24.47,,18.000,0.3 (0.01),2,0.35 (0.03),NGU22,1,,,NRAOVLA,+18 25 3.0256,-11 59 12.939,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.2626070,-11.9869280,19.2762620,0.3043810,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G19.2778+0.3049, 1,5(-1)->6(0)_A+,G19.485+0.151,G19.4959+0.1154,,15.0000000000,276.5381690,-11.8810510,19.4957560,0.1153830,,,,121.12,,18.000,5.1 (0.12),2,5.59 (0.23),NGU22,1,,,NRAOVLA,+18 26 9.1606,-11 52 51.784,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.5381690,-11.8810510,19.4957560,0.1153830,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G19.4958+0.1154, 1,5(-1)->6(0)_A+,G19.364-0.030,G19.3646-0.0304,,15.0000000000,276.6073010,-12.0649140,19.3646380,-0.0301750,,,,25.18,,18.000,33.32 (0.37),2,35.63 (0.7),NGU22,1,,,NRAOVLA,+18 26 25.7522,-12 03 53.691,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.6073010,-12.0649140,19.3646380,-0.0301750,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G19.3647-0.0304, 1,5(-1)->6(0)_A+,G19.310+0.065,G19.3125+0.0671,,15.0000000000,276.4937240,-12.0662910,19.3116230,0.0674340,,,,32.56,,18.000,1.88 (0.02),2,1.99 (0.04),NGU22,1,,,NRAOVLA,+18 25 58.4937,-12 03 58.647,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.4937240,-12.0662910,19.3116230,0.0674340,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G19.3099+0.0646, 1,5(-1)->6(0)_A+,G19.485+0.151,G19.4710+0.1728,,15.0000000000,276.4742700,-11.8762840,19.4708020,0.1729170,,,,14.57,,18.000,0.48 (0.03),2,0.72 (0.07),NGU22,1,,,NRAOVLA,+18 25 53.8247,-11 52 34.624,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.4742700,-11.8762840,19.4708020,0.1729170,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G19.4726+0.1699, 1,5(-1)->6(0)_A+,G19.485+0.151,G19.4724+0.1697,,15.0000000000,276.4779070,-11.8761680,19.4725660,0.1698230,,,,21.59,,18.000,8.87 (0.13),2,9.57 (0.24),NGU22,1,,,NRAOVLA,+18 25 54.6976,-11 52 34.205,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.4779070,-11.8761680,19.4725660,0.1698230,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G19.4726+0.1699, 1,5(-1)->6(0)_A+,G20.718-0.359,G20.7197-0.3472,,15.0000000000,277.5362030,-11.0126200,20.7193640,-0.3469940,,,,56.16,,18.000,0.39 (0.02),2,0.34 (0.03),NGU22,1,,,NRAOVLA,+18 30 8.6888,-11 00 45.431,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,277.5362030,-11.0126200,20.7193640,-0.3469940,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G20.7194-0.3470, 1,5(-1)->6(0)_A+,G20.764-0.059,G20.7620-0.0639,,15.0000000000,277.3007520,-10.8432010,20.7622640,-0.0636080,,,,57.42,,18.000,1.02 (0.02),2,1.14 (0.04),NGU22,1,,,NRAOVLA,+18 29 12.1806,-10 50 35.523,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,277.3007520,-10.8432010,20.7622640,-0.0636080,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G20.7620-0.0634, 1,5(-1)->6(0)_A+,G20.734-0.059,G20.7327-0.0595,,15.0000000000,277.2830820,-10.8675600,20.7326330,-0.0595410,,,,60.66,,18.000,0.89 (0.02),2,0.94 (0.04),NGU22,1,,,NRAOVLA,+18 29 7.9396,-10 52 3.217,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,277.2830820,-10.8675600,20.7326330,-0.0595410,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G20.7338-0.0592, 1,5(-1)->6(0)_A+,G20.081-0.136,G20.0815-0.1354,,15.0000000000,277.0428320,-11.4795510,20.0811850,-0.1350570,,,,43.53,,18.000,1.51 (0.02),2,1.55 (0.03),NGU22,1,,,NRAOVLA,+18 28 10.2796,-11 28 46.385,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,277.0428320,-11.4795510,20.0811850,-0.1350570,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G20.0816-0.1355, 1,5(-1)->6(0)_A+,G20.237+0.065,G20.2391+0.0646,,15.0000000000,276.9371610,-11.2466570,20.2392010,0.0649520,,,,60.64,,18.000,3.46 (0.04),2,3.63 (0.07),NGU22,1,,,NRAOVLA,+18 27 44.9187,-11 14 47.967,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.9371610,-11.2466570,20.2392010,0.0649520,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G20.2370+0.0654, 1,5(-1)->6(0)_A+,G20.237+0.065,G20.2370+0.0653,,15.0000000000,276.9355870,-11.2484010,20.2369390,0.0655070,,,,73.06,,18.000,18.21 (0.19),2,19.08 (0.35),NGU22,1,,,NRAOVLA,+18 27 44.541,-11 14 54.244,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.9355870,-11.2484010,20.2369390,0.0655070,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G20.2370+0.0654, 1,5(-1)->6(0)_A+,G20.364-0.013,G20.3634-0.0132,,15.0000000000,277.0661800,-11.1726520,20.3635620,-0.0126860,,,,56.16,,18.000,2.62 (0.04),2,2.76 (0.07),NGU22,1,,,NRAOVLA,+18 28 15.8831,-11 10 21.548,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,277.0661800,-11.1726520,20.3635620,-0.0126860,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G20.3639-0.0126, 1,5(-1)->6(0)_A+,G20.926-0.050,G20.9266-0.0500,,15.0000000000,277.3655950,-10.6913090,20.9263730,-0.0495650,,,,25.9,,18.000,2.65 (0.05),2,2.86 (0.09),NGU22,1,,,NRAOVLA,+18 29 27.7427,-10 41 28.712,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,277.3655950,-10.6913090,20.9263730,-0.0495650,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G20.9264-0.0497, 1,5(-1)->6(0)_A+,G20.963-0.075,G20.9627-0.0750,,15.0000000000,277.4055080,-10.6703740,20.9631120,-0.0746030,,,,34.54,,18.000,1.16 (0.03),2,1.37 (0.06),NGU22,1,,,NRAOVLA,+18 29 37.322,-10 40 13.348,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,277.4055080,-10.6703740,20.9631120,-0.0746030,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G20.9633-0.0746, 1,5(-1)->6(0)_A+,G20.441+0.322,G20.4419+0.3222,,15.0000000000,276.8007630,-10.9480260,20.4412470,0.3223900,,,,-2.73,,18.000,0.51 (0.02),2,0.6 (0.03),NGU22,1,,,NRAOVLA,+18 27 12.1831,-10 56 52.892,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,276.8007630,-10.9480260,20.4412470,0.3223900,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G20.4412+0.3224, 1,5(-1)->6(0)_A+,G20.731-0.160,G20.7308-0.1583,,15.0000000000,277.3710080,-10.9151180,20.7305650,-0.1580930,,,,55.62,,18.000,0.97 (0.02),2,1.1 (0.03),NGU22,1,,,NRAOVLA,+18 29 29.0419,-10 54 54.426,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,277.3710080,-10.9151180,20.7305650,-0.1580930,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G20.7306-0.1581, 1,5(-1)->6(0)_A+,G20.681-0.141,G20.6818-0.1469,,15.0000000000,277.3378750,-10.9533340,20.6816190,-0.1470020,,,,46.44,,18.000,0.18 (0.02),2,0.21 (0.03),NGU22,1,,,NRAOVLA,+18 29 21.09,-10 57 12.004,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,277.3378750,-10.9533340,20.6816190,-0.1470020,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G20.6816-0.1470, 1,5(-1)->6(0)_A+,G21.407-0.254,G21.4087-0.2539,,15.0000000000,277.7762570,-10.3605390,21.4065620,-0.2541240,,,,88.89,,18.000,11.37 (0.25),2,13.09 (0.49),NGU22,1,,,NRAOVLA,+18 31 6.3016,-10 21 37.941,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,277.7762570,-10.3605390,21.4065620,-0.2541240,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G21.4068-0.2541, 1,5(-1)->6(0)_A+,G21.563-0.031,G21.5621-0.0329,,15.0000000000,277.6500220,-10.1198630,21.5623930,-0.0325990,,,,117.17,,18.000,8.8 (0.19),2,9.9 (0.37),NGU22,1,,,NRAOVLA,+18 30 36.0052,-10 07 11.508,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,277.6500220,-10.1198630,21.5623930,-0.0325990,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G21.5609-0.0298, 1,5(-1)->6(0)_A+,G21.848-0.240,G21.8483-0.2400,,15.0000000000,277.9712500,-9.9626370,21.8481230,-0.2402760,,,,81.88,,18.000,0.54 (0.02),2,0.61 (0.04),NGU22,1,,,NRAOVLA,+18 31 53.1,-09 57 45.495,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,277.9712500,-9.9626370,21.8481230,-0.2402760,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G21.8481-0.2401, 1,5(-1)->6(0)_A+,G21.880+0.014,G21.8802+0.0142,,15.0000000000,277.7570050,-9.8170140,21.8796140,0.0142070,,,,20.15,,18.000,1.72 (0.05),2,1.91 (0.09),NGU22,1,,,NRAOVLA,+18 31 1.6812,-09 49 1.252,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,277.7570050,-9.8170140,21.8796140,0.0142070,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G21.8801+0.0140, 1,5(-1)->6(0)_A+,G21.386-0.253,G21.3872-0.2532,,15.0000000000,277.7661530,-10.3776900,21.3867580,-0.2532490,,,,87.08,,18.000,0.97 (0.03),2,1.21 (0.06),NGU22,1,,,NRAOVLA,+18 31 3.8767,-10 22 39.683,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,277.7661530,-10.3776900,21.3867580,-0.2532490,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G21.3858-0.2534, 1,5(-1)->6(0)_A+,G22.039+0.222,G22.0384+0.2225,,15.0000000000,277.6443130,-9.5798470,22.0384120,0.2224640,,,,54.36,,18.000,9.39 (0.21),2,10.38 (0.39),NGU22,1,,,NRAOVLA,+18 30 34.6352,-09 34 47.448,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,277.6443130,-9.5798470,22.0384120,0.2224640,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G22.0386+0.2223, 1,5(-1)->6(0)_A+,G22.335-0.155,G22.3349-0.1545,,15.0000000000,278.1224170,-9.4916260,22.3346870,-0.1547810,,,,35.43,,18.000,24.61 (0.42),2,26.49 (0.79),NGU22,1,,,NRAOVLA,+18 32 29.3801,-09 29 29.852,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.1224170,-9.4916260,22.3346870,-0.1547810,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G22.3348-0.1549, 1,5(-1)->6(0)_A+,G22.356+0.066,G22.3564+0.0663,,15.0000000000,277.9336200,-9.3702190,22.3562890,0.0664890,,,,80.26,,18.000,9.59 (0.16),2,10.65 (0.31),NGU22,1,,,NRAOVLA,+18 31 44.0687,-09 22 12.787,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,277.9336200,-9.3702190,22.3562890,0.0664890,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G22.3563+0.0663, 1,5(-1)->6(0)_A+,G22.435-0.169,G22.4356-0.1684,,15.0000000000,278.1824940,-9.4091520,22.4352080,-0.1692600,,,,29.32,,18.000,12.54 (0.21),2,13.6 (0.39),NGU22,1,,,NRAOVLA,+18 32 43.7986,-09 24 32.946,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.1824940,-9.4091520,22.4352080,-0.1692600,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G22.4352-0.1694, 1,5(-1)->6(0)_A+,G22.949+0.044,G22.9647+0.0463,,15.0000000000,278.2360820,-8.8397360,22.9647390,0.0466790,,,,35.97,,18.000,0.51 (0.03),2,0.65 (0.06),NGU22,1,,,NRAOVLA,+18 32 56.6597,-08 50 23.051,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.2360820,-8.8397360,22.9647390,0.0466790,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G22.9647+0.0467, 1,5(-1)->6(0)_A+,G23.425-0.219,G23.4215-0.2341,,15.0000000000,278.7011500,-8.5642210,23.4211760,-0.2342340,,,,104.62,,18.000,0.44 (0.02),2,0.47 (0.04),NGU22,1,,,NRAOVLA,+18 34 48.2759,-08 33 51.194,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.7011500,-8.5642210,23.4211760,-0.2342340,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G23.4200-0.2354, 1,5(-1)->6(0)_A+,G23.484+0.097,G23.4838+0.0963,,15.0000000000,278.4334990,-8.3562970,23.4837100,0.0965350,,,,88.1,,18.000,7.1 (0.02),2,7.15 (0.04),NGU22,1,,,NRAOVLA,+18 33 44.0397,-08 21 22.668,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.4334990,-8.3562970,23.4837100,0.0965350,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G23.4840+0.0968, 1,5(-1)->6(0)_A+,G23.657-0.127,G23.6566-0.1273,,15.0000000000,278.7147850,-8.3059160,23.6566740,-0.1272560,,,,82.4,,18.000,14.92 (0.06),2,15.04 (0.11),NGU22,1,,,NRAOVLA,+18 34 51.5484,-08 18 21.299,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.7147850,-8.3059160,23.6566740,-0.1272560,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G23.6567-0.1273, 1,5(-1)->6(0)_A+,G23.706-0.198,G23.7066-0.1985,,15.0000000000,278.8015010,-8.2944190,23.7063870,-0.1981350,,,,76.22,,18.000,17.68 (0.12),2,17.82 (0.22),NGU22,1,,,NRAOVLA,+18 35 12.3602,-08 17 39.907,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.8015010,-8.2944190,23.7063870,-0.1981350,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G23.7065-0.1981, 1,5(-1)->6(0)_A+,G23.818+0.384,G23.8181+0.3839,,15.0000000000,278.3315910,-7.9272010,23.8179130,0.3839560,,,,76.22,,18.000,0.58 (0.02),2,0.65 (0.03),NGU22,1,,,NRAOVLA,+18 33 19.5819,-07 55 37.923,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.3315910,-7.9272010,23.8179130,0.3839560,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G23.8179+0.3841, 1,5(-1)->6(0)_A+,G23.901+0.066,G23.9009+0.0763,,15.0000000000,278.6455660,-7.9952090,23.9009070,0.0766670,,,,35.8,,18.000,1.32 (0.02),2,1.37 (0.03),NGU22,1,,,NRAOVLA,+18 34 34.9359,-07 59 42.752,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.6455660,-7.9952090,23.9009070,0.0766670,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G23.9010+0.0768, 1,5(-1)->6(0)_A+,G23.901+0.066,G23.8853+0.0597,,15.0000000000,278.6536110,-8.0168000,23.8854130,0.0596500,,,,44.8,,18.000,2.39 (0.03),2,2.48 (0.05),NGU22,1,,,NRAOVLA,+18 34 36.8666,-08 01 0.479,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.6536110,-8.0168000,23.8854130,0.0596500,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G23.8854+0.0597, 1,5(-1)->6(0)_A+,G23.901+0.066,G23.8987+0.0641,,15.0000000000,278.6555790,-8.0031000,23.8984700,0.0642310,,,,42.64,,18.000,0.35 (0.01),2,0.32 (0.02),NGU22,1,,,NRAOVLA,+18 34 37.339,-08 00 11.159,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.6555790,-8.0031000,23.8984700,0.0642310,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G23.8985+0.0642, 1,5(-1)->6(0)_A+,G23.966-0.110,G23.9662-0.1092,,15.0000000000,278.8425280,-8.0229750,23.9660620,-0.1092540,,,,70.72,,18.000,18.32 (0.08),2,18.36 (0.14),NGU22,1,,,NRAOVLA,+18 35 22.2067,-08 01 22.711,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.8425280,-8.0229750,23.9660620,-0.1092540,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G23.9661-0.1098, 1,5(-1)->6(0)_A+,G23.996-0.100,G23.9862-0.0890,,15.0000000000,278.8337350,-7.9958830,23.9861080,-0.0890560,,,,65.14,,18.000,2.82 (0.01),2,2.91 (0.03),NGU22,1,,,NRAOVLA,+18 35 20.0965,-07 59 45.179,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.8337350,-7.9958830,23.9861080,-0.0890560,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G23.9861-0.0890, 1,5(-1)->6(0)_A+,G23.003+0.125,G23.0042+0.1247,,15.0000000000,278.1842400,-8.7689990,23.0038360,0.1247810,,,,111.06,,18.000,2.77 (0.02),2,2.79 (0.04),NGU22,1,,,NRAOVLA,+18 32 44.2175,-08 46 8.397,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.1842400,-8.7689990,23.0038360,0.1247810,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G23.0033+0.1246, 1,5(-1)->6(0)_A+,G23.996-0.100,G23.9964-0.0995,,15.0000000000,278.8481500,-7.9916000,23.9964800,-0.0997580,,,,66.58,,18.000,0.31 (0.01),2,0.29 (0.02),NGU22,1,,,NRAOVLA,+18 35 23.5561,-07 59 29.759,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.8481500,-7.9916000,23.9964800,-0.0997580,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G23.9958-0.0997, 1,5(-1)->6(0)_A+,G23.010-0.411,G23.0099-0.4108,,15.0000000000,278.6678510,-9.0106370,23.0097570,-0.4106140,,,,74.8,,18.000,479.22 (3.06),2,487.9 (5.49),NGU22,1,,,NRAOVLA,+18 34 40.2842,-09 00 38.293,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.6678510,-9.0106370,23.0097570,-0.4106140,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G23.0097-0.4106, 1,5(-1)->6(0)_A+,G23.126+0.395,G23.1260+0.3950,,15.0000000000,277.9989840,-8.5358670,23.1260060,0.3949080,,,,13.64,,18.000,0.94 (0.02),2,1 (0.04),NGU22,1,,,NRAOVLA,+18 31 59.7561,-08 32 9.12,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,277.9989840,-8.5358670,23.1260060,0.3949080,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G23.1260+0.3949, 1,5(-1)->6(0)_A+,G23.207-0.378,G23.2066-0.3778,,15.0000000000,278.7299400,-8.8208100,23.2065100,-0.3776490,,,,81.52,,18.000,31.82 (0.19),2,32.38 (0.35),NGU22,1,,,NRAOVLA,+18 34 55.1856,-08 49 14.917,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.7299400,-8.8208100,23.2065100,-0.3776490,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G23.2073-0.3780, 1,5(-1)->6(0)_A+,G23.257-0.240,G23.2544-0.2407,,15.0000000000,278.6300840,-8.7132830,23.2565050,-0.2405270,,,,63.92,,18.000,5.28 (0.03),2,5.36 (0.05),NGU22,1,,,NRAOVLA,+18 34 31.2202,-08 42 47.817,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.6300840,-8.7132830,23.2565050,-0.2405270,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G23.2569-0.2405, 1,5(-1)->6(0)_A+,G23.365-0.290,G23.3649-0.2906,,15.0000000000,278.7254620,-8.6403950,23.3646270,-0.2906490,,,,82.6,,18.000,0.84 (0.02),2,0.85 (0.03),NGU22,1,,,NRAOVLA,+18 34 54.1109,-08 38 25.422,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.7254620,-8.6403950,23.3646270,-0.2906490,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G23.3646-0.2900, 1,5(-1)->6(0)_A+,G23.389+0.185,G23.3892+0.1854,,15.0000000000,278.3096940,-8.3994790,23.3888990,0.1852920,,,,75.32,,18.000,31.66 (0.2),2,31.99 (0.36),NGU22,1,,,NRAOVLA,+18 33 14.3266,-08 23 58.124,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.3096940,-8.3994790,23.3888990,0.1852920,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G23.3891+0.1853, 1,5(-1)->6(0)_A+,G23.437-0.184,G23.4352-0.1846,,15.0000000000,278.6635530,-8.5276310,23.4365310,-0.1843810,,,,102.82,,18.000,49.9 (0.31),2,51.46 (0.57),NGU22,1,,,NRAOVLA,+18 34 39.2527,-08 31 39.47,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.6635530,-8.5276310,23.4365310,-0.1843810,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G23.4370-0.1831, 1,5(-1)->6(0)_A+,G23.437-0.184,G23.4400-0.1822,,15.0000000000,278.6632280,-8.5237820,23.4397990,-0.1823230,,,,97.42,,18.000,39.02 (0.11),2,39.14 (0.2),NGU22,1,,,NRAOVLA,+18 34 39.1747,-08 31 25.617,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.6632280,-8.5237820,23.4397990,-0.1823230,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G23.4370-0.1831, 1,5(-1)->6(0)_A+,G24.676-0.151,G24.6755-0.1500,,15.0000000000,279.2081600,-7.4118800,24.6753270,-0.1499800,,,,115.73,,18.000,1.46 (0.03),2,1.49 (0.05),NGU22,1,,,NRAOVLA,+18 36 49.9584,-07 24 42.769,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.2081600,-7.4118800,24.6753270,-0.1499800,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G24.6755-0.1515, 1,5(-1)->6(0)_A+,G24.850+0.087,G24.8503+0.0871,,15.0000000000,279.0765710,-7.1475300,24.8501070,0.0874440,,,,110.15,,18.000,14.16 (0.07),2,14.16 (0.13),NGU22,1,,,NRAOVLA,+18 36 18.3771,-07 08 51.108,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.0765710,-7.1475300,24.8501070,0.0874440,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G24.8501+0.0874, 1,5(-1)->6(0)_A+,G24.942+0.075,G24.9199+0.0882,,15.0000000000,279.1080820,-7.0855080,24.9195610,0.0881890,,,,53.24,,18.000,7.9 (0.03),2,7.86 (0.06),NGU22,1,,,NRAOVLA,+18 36 25.9396,-07 05 7.83,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.1080820,-7.0855080,24.9195610,0.0881890,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G24.9196+0.0882, 1,5(-1)->6(0)_A+,G24.942+0.075,G24.9428+0.0736,,15.0000000000,279.1315170,-7.0713700,24.9428070,0.0740340,,,,46.58,,18.000,1.68 (0.02),2,1.68 (0.04),NGU22,1,,,NRAOVLA,+18 36 31.564,-07 04 16.933,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.1315170,-7.0713700,24.9428070,0.0740340,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G24.9429+0.0744, 1,5(-1)->6(0)_A+,G24.297-0.153,G24.2984-0.1521,,15.0000000000,279.0349350,-7.7479740,24.2979130,-0.1519720,,,,100.98,,18.000,1.05 (0.01),2,1.1 (0.03),NGU22,1,,,NRAOVLA,+18 36 8.3845,-07 44 52.708,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.0349350,-7.7479740,24.2979130,-0.1519720,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G24.2948-0.1533, 1,5(-1)->6(0)_A+,G24.369-0.159,G24.3741-0.1584,,15.0000000000,279.0762910,-7.6831360,24.3743340,-0.1585530,,,,55.26,,18.000,2.19 (0.02),2,2.18 (0.04),NGU22,1,,,NRAOVLA,+18 36 18.3098,-07 40 59.29,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.0762910,-7.6831360,24.3743340,-0.1585530,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G24.3743-0.1586, 1,5(-1)->6(0)_A+,G24.632+0.173,G24.6317+0.1722,,15.0000000000,278.8990950,-7.3024580,24.6315600,0.1725290,,,,114.28,,18.000,1.8 (0.02),2,1.81 (0.04),NGU22,1,,,NRAOVLA,+18 35 35.7828,-07 18 8.85,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.8990950,-7.3024580,24.6315600,0.1725290,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G24.6325+0.1725, 1,5(-1)->6(0)_A+,G24.546-0.272,G24.5463-0.2722,,15.0000000000,279.2574840,-7.5828090,24.5459730,-0.2719460,,,,89.43,,18.000,0.36 (0.02),2,0.35 (0.03),NGU22,1,,,NRAOVLA,+18 37 1.7962,-07 34 58.111,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.2574840,-7.5828090,24.5459730,-0.2719460,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G24.5457-0.2723, 1,5(-1)->6(0)_A+,G24.257-0.150,G24.2574-0.1500,,15.0000000000,279.0138910,-7.7834140,24.2568540,-0.1497530,,,,89.43,,18.000,0.35 (0.02),2,0.38 (0.04),NGU22,1,,,NRAOVLA,+18 36 3.3339,-07 47 0.291,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.0138910,-7.7834140,24.2568540,-0.1497530,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G24.2569-0.1498, 1,5(-1)->6(0)_A+,G24.662-0.079,G24.6623-0.0792,,15.0000000000,279.1386430,-7.3910470,24.6621490,-0.0791790,,,,49.46,,18.000,0.24 (0.02),2,0.2 (0.04),NGU22,1,,,NRAOVLA,+18 36 33.2743,-07 23 27.768,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.1386430,-7.3910470,24.6621490,-0.0791790,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G24.6621-0.0792, 1,5(-1)->6(0)_A+,G24.257-0.150,G24.2574-0.1500,,15.0000000000,279.0138910,-7.7834140,24.2568540,-0.1497530,,,,89.43,,18.000,0.35 (0.02),2,0.38 (0.04),NGU22,1,,,NRAOVLA,+18 36 3.3339,-07 47 0.291,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.0138910,-7.7834140,24.2568540,-0.1497530,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G24.2569-0.1498, 1,5(-1)->6(0)_A+,G24.942+0.075,G24.9220+0.0833,,15.0000000000,279.1135400,-7.0859170,24.9216880,0.0831900,,,,39.39,,18.000,0.3 (0.02),2,0.35 (0.04),NGU22,1,,,NRAOVLA,+18 36 27.2497,-07 05 9.302,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.1135400,-7.0859170,24.9216880,0.0831900,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G24.9215+0.0846, 1,5(-1)->6(0)_A+,G24.790+0.083,G24.7916+0.0815,,15.0000000000,279.0523130,-7.2030680,24.7897220,0.0832830,,,,113.36,,18.000,88.05 (0.41),2,88.38 (0.74),NGU22,1,,,NRAOVLA,+18 36 12.5551,-07 12 11.043,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.0523130,-7.2030680,24.7897220,0.0832830,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G24.7898+0.0832, 1,5(-1)->6(0)_A+,G24.676-0.151,G24.6740-0.1535,,15.0000000000,279.2107900,-7.4146740,24.6740440,-0.1535800,,,,113.57,,18.000,0.73 (0.02),2,0.87 (0.04),NGU22,1,,,NRAOVLA,+18 36 50.5896,-07 24 52.826,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.2107900,-7.4146740,24.6740440,-0.1535800,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G24.6755-0.1515, 1,5(-1)->6(0)_A+,G24.942+0.075,G24.9217+0.0832,,15.0000000000,279.1134750,-7.0859420,24.9216360,0.0832360,,,,39.38,,18.000,0.31 (0.02),2,0.35 (0.03),NGU22,1,,,NRAOVLA,+18 36 27.2339,-07 05 9.393,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.1134750,-7.0859420,24.9216360,0.0832360,0.018,,,,,0.18,1,D,,,G24.9215+0.0846, 1,5(-1)->6(0)_A+,G24.329+0.144,G24.3289+0.1437,,15.0000000000,278.7840600,-7.5845330,24.3286360,0.1439800,,,,110.15,,18.000,5.86 (0.03),2,5.9 (0.05),NGU22,1,,,NRAOVLA,+18 35 8.1744,-07 35 4.32,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.7840600,-7.5845330,24.3286360,0.1439800,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G24.3287+0.1440, 1,5(-1)->6(0)_A+,G24.461+0.198,G24.4609+0.1979,,15.0000000000,278.7970500,-7.4420070,24.4610930,0.1981560,,,,120.94,,18.000,7.82 (0.05),2,7.87 (0.09),NGU22,1,,,NRAOVLA,+18 35 11.2921,-07 26 31.224,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.7970500,-7.4420070,24.4610930,0.1981560,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G24.4612+0.1980, 1,5(-1)->6(0)_A+,G24.535+0.322,G24.5411+0.3121,,15.0000000000,278.7322100,-7.3184280,24.5411940,0.3121320,,,,109.96,,18.000,5.85 (0.04),2,5.88 (0.07),NGU22,1,,,NRAOVLA,+18 34 55.7305,-07 19 6.34,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.7322100,-7.3184280,24.5411940,0.3121320,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G24.5411+0.3121, 1,5(-1)->6(0)_A+,G24.497+0.115,G24.4981+0.1151,,15.0000000000,278.8882570,-7.4480240,24.4973720,0.1150950,,,,115,,18.000,0.17 (0.02),2,0.22 (0.04),NGU22,1,,,NRAOVLA,+18 35 33.1817,-07 26 52.888,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.8882570,-7.4480240,24.4973720,0.1150950,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G24.4974+0.1151, 1,5(-1)->6(0)_A+,G24.494-0.040,G24.4935-0.0382,,15.0000000000,279.0237950,-7.5222020,24.4933220,-0.0383470,,,,115.01,,18.000,24.2 (0.19),2,24.43 (0.35),NGU22,1,,,NRAOVLA,+18 36 5.7107,-07 31 19.929,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.0237950,-7.5222020,24.4933220,-0.0383470,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G24.4936-0.0389, 1,5(-1)->6(0)_A+,G24.499+0.054,G24.4974+0.0534,,15.0000000000,278.9431070,-7.4758170,24.4977160,0.0540210,,,,108.35,,18.000,0.22 (0.02),2,0.28 (0.03),NGU22,1,,,NRAOVLA,+18 35 46.3456,-07 28 32.943,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.9431070,-7.4758170,24.4977160,0.0540210,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G24.4986+0.0541, 1,5(-1)->6(0)_A+,G24.535+0.322,G24.5414+0.3118,,15.0000000000,278.7321990,-7.3185470,24.5410830,0.3120870,,,,109.97,,18.000,5.56 (0.04),2,5.57 (0.07),NGU22,1,,,NRAOVLA,+18 34 55.7277,-07 19 6.769,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,278.7321990,-7.3185470,24.5410830,0.3120870,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G24.5411+0.3121, 1,5(-1)->6(0)_A+,G25.920-0.141,G25.9203-0.1406,,15.0000000000,279.7752690,-6.3016850,25.9201060,-0.1406680,,,,113.75,,18.000,0.68 (0.02),2,0.78 (0.05),NGU22,1,,,NRAOVLA,+18 39 6.0646,-06 18 6.066,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.7752690,-6.3016850,25.9201060,-0.1406680,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G25.9205-0.1405, 1,5(-1)->6(0)_A+,G25.179+0.211,G25.1772+0.2111,,15.0000000000,279.1193330,-6.7989120,25.1792200,0.2100090,,,,114.12,,18.000,0.11 (0.01),2,0.09 (0.03),NGU22,1,,,NRAOVLA,+18 36 28.64,-06 47 56.083,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.1193330,-6.7989120,25.1792200,0.2100090,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G25.1792+0.2110, 1,5(-1)->6(0)_A+,G25.181+0.190,G25.1807+0.1892,,15.0000000000,279.1385380,-6.8062440,25.1814730,0.1897030,,,,100.44,,18.000,0.38 (0.02),2,0.44 (0.03),NGU22,1,,,NRAOVLA,+18 36 33.2492,-06 48 22.48,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.1385380,-6.8062440,25.1814730,0.1897030,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G25.1815+0.1897, 1,5(-1)->6(0)_A+,G25.227+0.289,G25.2256+0.2884,,15.0000000000,279.0707200,-6.7214700,25.2258030,0.2884810,,,,41.38,,18.000,0.18 (0.02),2,0.18 (0.04),NGU22,1,,,NRAOVLA,+18 36 16.9728,-06 43 17.291,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.0707200,-6.7214700,25.2258030,0.2884810,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G25.2274+0.2887, 1,5(-1)->6(0)_A+,G25.270-0.434,G25.2702-0.4337,,15.0000000000,279.7373340,-7.0137480,25.2700140,-0.4336630,,,,55.08,,18.000,2.5 (0.02),2,2.54 (0.03),NGU22,1,,,NRAOVLA,+18 38 56.9602,-07 00 49.493,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.7373340,-7.0137480,25.2700140,-0.4336630,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G25.2703-0.4336, 1,5(-1)->6(0)_A+,G25.382-0.181,G25.3821-0.1816,,15.0000000000,279.5634130,-6.7989220,25.3817170,-0.1817020,,,,60.47,,18.000,5.74 (0.04),2,5.85 (0.08),NGU22,1,,,NRAOVLA,+18 38 15.2191,-06 47 56.121,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.5634130,-6.7989220,25.3817170,-0.1817020,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G25.3817-0.1812, 1,5(-1)->6(0)_A+,G25.411+0.105,G25.4105+0.1045,,15.0000000000,279.3204750,-6.6419390,25.4104260,0.1047070,,,,96.98,,18.000,13.01 (0.04),2,13.07 (0.07),NGU22,1,,,NRAOVLA,+18 37 16.914,-06 38 30.979,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.3204750,-6.6419390,25.4104260,0.1047070,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G25.4106+0.1050, 1,5(-1)->6(0)_A+,G25.494+0.062,G25.4932+0.0614,,15.0000000000,279.3976220,-6.5870320,25.4943920,0.0618450,,,,103.68,,18.000,3.63 (0.04),2,3.69 (0.07),NGU22,1,,,NRAOVLA,+18 37 35.4293,-06 35 13.314,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.3976220,-6.5870320,25.4943920,0.0618450,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G25.4944+0.0618, 1,5(-1)->6(0)_A+,G25.613+0.226,G25.6133+0.2253,,15.0000000000,279.3059360,-6.4059950,25.6133790,0.2259040,,,,115.01,,18.000,0.73 (0.02),2,0.83 (0.05),NGU22,1,,,NRAOVLA,+18 37 13.4246,-06 24 21.581,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.3059360,-6.4059950,25.6133790,0.2259040,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G25.6132+0.2259, 1,5(-1)->6(0)_A+,G25.709+0.044,G25.7098+0.0441,,15.0000000000,279.5131900,-6.4042030,25.7095300,0.0437560,,,,95.54,,18.000,349.61 (4.21),2,353.06 (7.52),NGU22,1,,,NRAOVLA,+18 38 3.1657,-06 24 15.129,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.5131900,-6.4042030,25.7095300,0.0437560,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G25.7095+0.0438, 1,5(-1)->6(0)_A+,G25.805-0.041,G25.8026-0.0418,,15.0000000000,279.6325150,-6.3609430,25.8023780,-0.0417600,,,,90.86,,18.000,0.87 (0.06),2,1.21 (0.14),NGU22,1,,,NRAOVLA,+18 38 31.8035,-06 21 39.395,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.6325150,-6.3609430,25.8023780,-0.0417600,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G25.8053-0.0412, 1,5(-1)->6(0)_A+,G25.826-0.178,G25.8258-0.1781,,15.0000000000,279.7651880,-6.4031960,25.8252990,-0.1783060,,,,91.58,,18.000,75.22 (0.45),2,75.74 (0.8),NGU22,1,,,NRAOVLA,+18 39 3.6451,-06 24 11.506,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.7651880,-6.4031960,25.8252990,-0.1783060,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G25.8257-0.1780, 1,5(-1)->6(0)_A+,G25.838-0.378,G25.8348-0.3795,,15.0000000000,279.9494900,-6.4844210,25.8370470,-0.3783030,,,,-1.83,,18.000,0.6 (0.01),2,0.57 (0.02),NGU22,1,,,NRAOVLA,+18 39 47.8776,-06 29 3.917,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.9494900,-6.4844210,25.8370470,-0.3783030,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G25.8375-0.3780, 1,5(-1)->6(0)_A+,G26.545+0.417,G26.5451+0.4222,,15.0000000000,279.5601750,-5.4882540,26.5448030,0.4225410,,,,82.41,,18.000,3.42 (0.04),2,3.46 (0.07),NGU22,1,,,NRAOVLA,+18 38 14.442,-05 29 17.716,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.5601750,-5.4882540,26.5448030,0.4225410,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G26.5451+0.4226, 1,5(-1)->6(0)_A+,G26.527-0.267,G26.5270-0.2674,,15.0000000000,280.1676810,-5.8203520,26.5267360,-0.2669820,,,,104.22,,18.000,4.94 (0.02),2,4.94 (0.04),NGU22,1,,,NRAOVLA,+18 40 40.2435,-05 49 13.266,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.1676810,-5.8203520,26.5267360,-0.2669820,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G26.5269-0.2670, 1,5(-1)->6(0)_A+,G26.513-0.294,G26.5137-0.2929,,15.0000000000,280.1846610,-5.8439180,26.5135200,-0.2927900,,,,109.44,,18.000,0.79 (0.03),2,0.83 (0.05),NGU22,1,,,NRAOVLA,+18 40 44.3187,-05 50 38.105,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.1846610,-5.8439180,26.5135200,-0.2927900,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G26.5134-0.2939, 1,5(-1)->6(0)_A+,G26.555-0.303,G26.5517-0.3093,,15.0000000000,280.2168340,-5.8175010,26.5516590,-0.3091500,,,,107.1,,18.000,1.43 (0.02),2,1.39 (0.04),NGU22,1,,,NRAOVLA,+18 40 52.0401,-05 49 3.004,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.2168340,-5.8175010,26.5516590,-0.3091500,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G26.5517-0.3091, 1,5(-1)->6(0)_A+,G26.597-0.024,G26.5979-0.0236,,15.0000000000,279.9830090,-5.6458220,26.5977230,-0.0237020,,,,24.83,,18.000,12.45 (0.12),2,12.69 (0.21),NGU22,1,,,NRAOVLA,+18 39 55.9222,-05 38 44.959,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.9830090,-5.6458220,26.5977230,-0.0237020,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G26.5975-0.0238, 1,5(-1)->6(0)_A+,G26.602-0.220,G26.6006-0.2215,,15.0000000000,280.1606780,-5.7339570,26.6003520,-0.2212290,,,,114.83,,18.000,7.28 (0.05),2,7.3 (0.09),NGU22,1,,,NRAOVLA,+18 40 38.5626,-05 44 2.247,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.1606780,-5.7339570,26.6003520,-0.2212290,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G26.6018-0.2206, 1,5(-1)->6(0)_A+,G26.647+0.017,G26.6479+0.0166,,15.0000000000,279.9696020,-5.5826510,26.6477590,0.0171010,,,,109.07,,18.000,2.56 (0.02),2,2.58 (0.03),NGU22,1,,,NRAOVLA,+18 39 52.7044,-05 34 57.545,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.9696020,-5.5826510,26.6477590,0.0171010,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G26.6453+0.0163, 1,5(-1)->6(0)_A+,G26.689+0.035,G26.6860+0.0341,,15.0000000000,279.9713830,-5.5406640,26.6858920,0.0347630,,,,85.67,,18.000,0.32 (0.02),2,0.31 (0.03),NGU22,1,,,NRAOVLA,+18 39 53.1319,-05 32 26.392,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.9713830,-5.5406640,26.6858920,0.0347630,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G26.6859+0.0348, 1,5(-1)->6(0)_A+,G26.109-0.094,G26.1090-0.0938,,15.0000000000,279.8202300,-6.1123500,26.1088630,-0.0935900,,,,25.9,,18.000,0.48 (0.02),2,0.5 (0.04),NGU22,1,,,NRAOVLA,+18 39 16.8551,-06 06 44.459,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,279.8202300,-6.1123500,26.1088630,-0.0935900,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G26.1094-0.0936, 1,5(-1)->6(0)_A+,G27.757+0.050,G27.7570+0.0500,,15.0000000000,280.4498770,-4.5813210,27.7569990,0.0502540,,,,99.1,,18.000,1.5 (0.02),2,1.61 (0.04),NGU22,1,,,NRAOVLA,+18 41 47.9705,-04 34 52.755,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.4498770,-4.5813210,27.7569990,0.0502540,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G27.7570+0.0502, 1,5(-1)->6(0)_A+,G27.783-0.260,G27.7827-0.2590,,15.0000000000,280.7371600,-4.6996810,27.7826960,-0.2585180,,,,98.19,,18.000,3.77 (0.04),2,3.62 (0.07),NGU22,1,,,NRAOVLA,+18 42 56.9184,-04 41 58.852,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.7371600,-4.6996810,27.7826960,-0.2585180,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G27.7829-0.2583, 1,5(-1)->6(0)_A+,G27.784+0.057,G27.7848+0.0570,,15.0000000000,280.4565240,-4.5537100,27.7845820,0.0569950,,,,112.04,,18.000,2.76 (0.03),2,2.81 (0.05),NGU22,1,,,NRAOVLA,+18 41 49.5658,-04 33 13.355,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.4565240,-4.5537100,27.7845820,0.0569950,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G27.7845+0.0569, 1,5(-1)->6(0)_A+,G27.656+0.080,G27.6487+0.0931,,15.0000000000,280.3620840,-4.6576860,27.6490550,0.0931210,,,,36.24,,18.000,1.4 (0.03),2,1.46 (0.05),NGU22,1,,,NRAOVLA,+18 41 26.9002,-04 39 27.671,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.3620840,-4.6576860,27.6490550,0.0931210,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G27.6491+0.0931, 1,5(-1)->6(0)_A+,G27.011-0.039,G27.0091-0.0395,,15.0000000000,280.1869460,-5.2859350,27.0106230,-0.0393320,,,,-20.99,,18.000,1.77 (0.03),2,1.79 (0.06),NGU22,1,,,NRAOVLA,+18 40 44.867,-05 17 9.366,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.1869460,-5.2859350,27.0106230,-0.0393320,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G27.0106-0.0394, 1,5(-1)->6(0)_A+,G27.221+0.136,G27.2216+0.1362,,15.0000000000,280.1272430,-5.0181980,27.2214130,0.1361280,,,,118.33,,18.000,20.19 (0.08),2,20.28 (0.15),NGU22,1,,,NRAOVLA,+18 40 30.5384,-05 01 5.513,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.1272430,-5.0181980,27.2214130,0.1361280,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G27.2215+0.1361, 1,5(-1)->6(0)_A+,G27.220+0.260,G27.2175+0.2605,,15.0000000000,280.0154860,-4.9628200,27.2196480,0.2604610,,,,9.27,,18.000,5.54 (0.05),2,5.6 (0.09),NGU22,1,,,NRAOVLA,+18 40 3.7166,-04 57 46.152,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.0154860,-4.9628200,27.2196480,0.2604610,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G27.2198+0.2605, 1,5(-1)->6(0)_A+,G27.284+0.149,G27.2862+0.1507,,15.0000000000,280.1437740,-4.9539680,27.2860540,0.1509010,,,,34.63,,18.000,28.35 (0.15),2,28.61 (0.27),NGU22,1,,,NRAOVLA,+18 40 34.5057,-04 57 14.285,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.1437740,-4.9539680,27.2860540,0.1509010,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G27.2860+0.1509, 1,5(-1)->6(0)_A+,G27.256+0.136,G27.2552+0.1361,,15.0000000000,280.1435230,-4.9879390,27.2557400,0.1355670,,,,37.69,,18.000,0.4 (0.02),2,0.41 (0.03),NGU22,1,,,NRAOVLA,+18 40 34.4456,-04 59 16.58,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.1435230,-4.9879390,27.2557400,0.1355670,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G27.2557+0.1356, 1,5(-1)->6(0)_A+,G27.367-0.165,G27.3654-0.1659,,15.0000000000,280.4626200,-5.0286430,27.3650460,-0.1656900,,,,100.71,,18.000,48.86 (0.22),2,49.29 (0.39),NGU22,1,,,NRAOVLA,+18 41 51.0289,-05 01 43.115,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.4626200,-5.0286430,27.3650460,-0.1656900,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G27.3650-0.1659, 1,5(-1)->6(0)_A+,G27.367-0.165,G27.3705-0.1647,,15.0000000000,280.4640110,-5.0239540,27.3698490,-0.1647770,,,,95.85,,18.000,0.44 (0.04),2,0.66 (0.08),NGU22,1,,,NRAOVLA,+18 41 51.3626,-05 01 26.235,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.4640110,-5.0239540,27.3698490,-0.1647770,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G27.3686-0.1636, 1,5(-1)->6(0)_A+,G27.563+0.080,G27.5640+0.0862,,15.0000000000,280.3291460,-4.7365210,27.5639380,0.0862300,,,,87,,18.000,0.69 (0.02),2,0.75 (0.04),NGU22,1,,,NRAOVLA,+18 41 18.9951,-04 44 11.474,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.3291460,-4.7365210,27.5639380,0.0862300,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G27.5639+0.0862, 1,5(-1)->6(0)_A+,G27.656+0.080,G27.6530+0.0711,,15.0000000000,280.3833570,-4.6642550,27.6529170,0.0712630,,,,74.22,,18.000,0.2 (0.02),2,0.2 (0.04),NGU22,1,,,NRAOVLA,+18 41 32.0056,-04 39 51.317,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.3833570,-4.6642550,27.6529170,0.0712630,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G27.6529+0.0713, 1,5(-1)->6(0)_A+,G28.609+0.017,G28.6079+0.0180,,15.0000000000,280.8688040,-3.8396110,28.6076660,0.0178560,,,,106.33,,18.000,2.77 (0.03),2,2.65 (0.05),NGU22,1,,,NRAOVLA,+18 43 28.513,-03 50 22.599,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.8688040,-3.8396110,28.6076660,0.0178560,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G28.6089+0.0171, 1,5(-1)->6(0)_A+,G28.700+0.406,G28.7002+0.4059,,15.0000000000,280.5647600,-3.5797830,28.7000380,0.4064870,,,,94.15,,18.000,0.45 (0.01),2,0.37 (0.02),NGU22,1,,,NRAOVLA,+18 42 15.5423,-03 34 47.218,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.5647600,-3.5797830,28.7000380,0.4064870,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G28.7011+0.4055, 1,5(-1)->6(0)_A+,G28.700+0.406,G28.7003+0.4060,,15.0000000000,280.5647200,-3.5797690,28.7000330,0.4065290,,,,94.19,,18.000,0.45 (0.01),2,0.4 (0.02),NGU22,1,,,NRAOVLA,+18 42 15.5327,-03 34 47.167,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.5647200,-3.5797690,28.7000330,0.4065290,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G28.7011+0.4055, 1,5(-1)->6(0)_A+,G28.817+0.365,G28.8175+0.3649,,15.0000000000,280.6556240,-3.4947880,28.8171010,0.3647000,,,,91.09,,18.000,5.43 (0.05),2,5.15 (0.09),NGU22,1,,,NRAOVLA,+18 42 37.3497,-03 29 41.235,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.6556240,-3.4947880,28.8171010,0.3647000,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G28.8171+0.3647, 1,5(-1)->6(0)_A+,G28.817+0.365,G28.8195+0.3543,,15.0000000000,280.6659280,-3.4977200,28.8191950,0.3542130,,,,86.82,,18.000,0.33 (0.01),2,0.34 (0.02),NGU22,1,,,NRAOVLA,+18 42 39.8226,-03 29 51.793,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.6659280,-3.4977200,28.8191950,0.3542130,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G28.8192+0.3542, 1,5(-1)->6(0)_A+,G28.833-0.253,G28.8322-0.2528,,15.0000000000,281.2127950,-3.7634340,28.8322370,-0.2526620,,,,91.81,,18.000,70.9 (0.74),2,67.31 (1.25),NGU22,1,,,NRAOVLA,+18 44 51.0707,-03 45 48.363,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.2127950,-3.7634340,28.8322370,-0.2526620,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G28.8322-0.2530, 1,5(-1)->6(0)_A+,G28.842+0.494,G28.8421+0.4938,,15.0000000000,280.5522690,-3.4135870,28.8421390,0.4935810,,,,87.85,,18.000,2.91 (0.02),2,2.81 (0.03),NGU22,1,,,NRAOVLA,+18 42 12.5445,-03 24 48.913,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.5522690,-3.4135870,28.8421390,0.4935810,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G28.8429+0.4938, 1,5(-1)->6(0)_A+,G28.833-0.253,G28.8481-0.2279,,15.0000000000,281.1976900,-3.7380340,28.8479510,-0.2276530,,,,102.82,,18.000,1.78 (0.04),2,1.81 (0.07),NGU22,1,,,NRAOVLA,+18 44 47.4455,-03 44 16.922,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.1976900,-3.7380340,28.8479510,-0.2276530,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G28.8480-0.2277, 1,5(-1)->6(0)_A+,G28.862+0.066,G28.8621+0.0660,,15.0000000000,280.9425750,-3.5915820,28.8619230,0.0657250,,,,104.89,,18.000,1.82 (0.03),2,1.75 (0.05),NGU22,1,,,NRAOVLA,+18 43 46.2179,-03 35 29.695,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.9425750,-3.5915820,28.8619230,0.0657250,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G28.8619+0.0657, 1,5(-1)->6(0)_A+,G28.928+0.019,G28.9289+0.0193,,15.0000000000,281.0146150,-3.5536340,28.9285300,0.0191080,,,,47.48,,18.000,0.26 (0.02),2,0.23 (0.03),NGU22,1,,,NRAOVLA,+18 44 3.5076,-03 33 13.082,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.0146150,-3.5536340,28.9285300,0.0191080,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G28.9284+0.0191, 1,5(-1)->6(0)_A+,G28.011-0.426,G28.0113-0.4263,,15.0000000000,280.9914920,-4.5733300,28.0109350,-0.4262530,,,,17,,18.000,4.69 (0.07),2,4.62 (0.12),NGU22,1,,,NRAOVLA,+18 43 57.958,-04 34 23.989,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.9914920,-4.5733300,28.0109350,-0.4262530,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G28.0110-0.4263, 1,5(-1)->6(0)_A+,G28.147-0.004,G28.1467-0.0045,,15.0000000000,280.6774670,-4.2597260,28.1467690,-0.0044430,,,,101.12,,18.000,28.34 (0.22),2,27.57 (0.39),NGU22,1,,,NRAOVLA,+18 42 42.592,-04 15 35.013,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.6774670,-4.2597260,28.1467690,-0.0044430,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G28.1467-0.0046, 1,5(-1)->6(0)_A+,G28.200-0.050,G28.2006-0.0495,,15.0000000000,280.7420320,-4.2325260,28.2003980,-0.0492720,,,,98.69,,18.000,2.19 (0.02),2,2.09 (0.04),NGU22,1,,,NRAOVLA,+18 42 58.0878,-04 13 57.092,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.7420320,-4.2325260,28.2003980,-0.0492720,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G28.2000-0.0495, 1,5(-1)->6(0)_A+,G28.295-0.377,G28.2817-0.3590,,15.0000000000,281.0552700,-4.3014800,28.2818150,-0.3586270,,,,41.41,,18.000,5.03 (0.06),2,4.77 (0.1),NGU22,1,,,NRAOVLA,+18 44 13.2647,-04 18 5.328,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.0552700,-4.3014800,28.2818150,-0.3586270,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G28.2819-0.3585, 1,5(-1)->6(0)_A+,G28.295-0.377,G28.3047-0.3877,,15.0000000000,281.0915140,-4.2945190,28.3045170,-0.3875980,,,,81.83,,18.000,26.79 (0.29),2,25.41 (0.49),NGU22,1,,,NRAOVLA,+18 44 21.9633,-04 17 40.267,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.0915140,-4.2945190,28.3045170,-0.3875980,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G28.3050-0.3875, 1,5(-1)->6(0)_A+,G28.295-0.377,G28.3047-0.3877,,15.0000000000,281.0915150,-4.2945200,28.3045170,-0.3875990,,,,82.19,,18.000,20.67 (0.22),2,19.56 (0.37),NGU22,1,,,NRAOVLA,+18 44 21.9635,-04 17 40.272,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.0915150,-4.2945200,28.3045170,-0.3875990,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G28.3050-0.3875, 1,5(-1)->6(0)_A+,G28.321-0.011,G28.3211-0.0110,,15.0000000000,280.7629700,-4.1074700,28.3211680,-0.0106730,,,,104.62,,18.000,2.63 (0.03),2,2.48 (0.05),NGU22,1,,,NRAOVLA,+18 43 3.1127,-04 06 26.891,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.7629700,-4.1074700,28.3211680,-0.0106730,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G28.3210-0.0108, 1,5(-1)->6(0)_A+,G28.397+0.078,G28.3972+0.0803,,15.0000000000,280.7165840,-3.9984660,28.3969600,0.0803110,,,,71.44,,18.000,16.7 (0.15),2,15.9 (0.26),NGU22,1,,,NRAOVLA,+18 42 51.9801,-03 59 54.478,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.7165840,-3.9984660,28.3969600,0.0803110,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G28.3970+0.0803, 1,5(-1)->6(0)_A+,G28.525+0.127,G28.5228+0.1270,,15.0000000000,280.7328030,-3.8654010,28.5227020,0.1267550,,,,39.48,,18.000,2.92 (0.02),2,2.75 (0.04),NGU22,1,,,NRAOVLA,+18 42 55.8728,-03 51 55.444,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.7328030,-3.8654010,28.5227020,0.1267550,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G28.5227+0.1267, 1,5(-1)->6(0)_A+,G28.525+0.127,G28.5322+0.1287,,15.0000000000,280.7353830,-3.8559760,28.5322610,0.1287750,,,,27.03,,18.000,2.04 (0.02),2,2 (0.04),NGU22,1,,,NRAOVLA,+18 42 56.4918,-03 51 21.513,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,280.7353830,-3.8559760,28.5322610,0.1287750,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G28.5323+0.1287, 1,5(-1)->6(0)_A+,G29.281-0.330,G29.2815-0.3295,,15.0000000000,281.4869390,-3.3989800,29.2814150,-0.3296920,,,,92.26,,18.000,2.95 (0.03),2,2.76 (0.05),NGU22,1,,,NRAOVLA,+18 45 56.8654,-03 23 56.327,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.4869390,-3.3989800,29.2814150,-0.3296920,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G29.2814-0.3297, 1,5(-1)->6(0)_A+,G29.319-0.162,G29.3197-0.1619,,15.0000000000,281.3548300,-3.2880150,29.3199360,-0.1616960,,,,48.83,,18.000,4.68 (0.04),2,4.47 (0.07),NGU22,1,,,NRAOVLA,+18 45 25.1593,-03 17 16.853,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.3548300,-3.2880150,29.3199360,-0.1616960,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G29.3199-0.1617, 1,5(-1)->6(0)_A+,G29.574+0.118,G29.5809+0.1320,,15.0000000000,281.2123620,-2.9216770,29.5808880,0.1321490,,,,31.88,,18.000,0.52 (0.01),2,0.54 (0.02),NGU22,1,,,NRAOVLA,+18 44 50.9669,-02 55 18.038,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.2123620,-2.9216770,29.5808880,0.1321490,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G29.5809+0.1321, 1,5(-1)->6(0)_A+,G29.594-0.617,G29.6032-0.6250,,15.0000000000,281.8975560,-3.2472330,29.6034990,-0.6252180,,,,81.74,,18.000,1.27 (0.02),2,1.17 (0.03),NGU22,1,,,NRAOVLA,+18 47 35.4134,-03 14 50.039,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.8975560,-3.2472330,29.6034990,-0.6252180,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G29.6035-0.6252, 1,5(-1)->6(0)_A+,G29.862-0.045,G29.8621-0.0441,,15.0000000000,281.4982150,-2.7517860,29.8623930,-0.0442880,,,,101.3,,18.000,83.65 (0.82),2,78.17 (1.38),NGU22,1,,,NRAOVLA,+18 45 59.5716,-02 45 6.429,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.4982150,-2.7517860,29.8623930,-0.0442880,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G29.8624-0.0442, 1,5(-1)->6(0)_A+,G29.915-0.043,G29.9157-0.0236,,15.0000000000,281.5040530,-2.6949230,29.9156470,-0.0235200,,,,104.3,,18.000,2.44 (0.06),2,2.58 (0.11),NGU22,1,,,NRAOVLA,+18 46 0.9726,-02 41 41.724,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.5040530,-2.6949230,29.9156470,-0.0235200,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G29.9156-0.0234, 1,5(-1)->6(0)_A+,G29.956-0.016,G29.9556-0.0156,,15.0000000000,281.5156330,-2.6562070,29.9553750,-0.0161390,,,,95.99,,18.000,135.71 (1.21),2,129.12 (2.05),NGU22,1,,,NRAOVLA,+18 46 3.7519,-02 39 22.346,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.5156330,-2.6562070,29.9553750,-0.0161390,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G29.9556-0.0161, 1,5(-1)->6(0)_A+,G29.961-0.068,G29.9609-0.0675,,15.0000000000,281.5640450,-2.6746920,29.9610020,-0.0676050,,,,100.27,,18.000,3.85 (0.08),2,3.46 (0.14),NGU22,1,,,NRAOVLA,+18 46 15.3708,-02 40 28.89,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.5640450,-2.6746920,29.9610020,-0.0676050,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G29.9610-0.0676, 1,5(-1)->6(0)_A+,G29.975-0.047,G29.9781-0.0478,,15.0000000000,281.5540400,-2.6504020,29.9780520,-0.0476260,,,,102.96,,18.000,31.12 (0.26),2,29.2 (0.44),NGU22,1,,,NRAOVLA,+18 46 12.9696,-02 39 1.448,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.5540400,-2.6504020,29.9780520,-0.0476260,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G29.9754-0.0474, 1,5(-1)->6(0)_A+,G30.589-0.043,G30.5891-0.0424,,15.0000000000,281.8286590,-2.1046530,30.5888740,-0.0427210,,,,42.99,,18.000,5.3 (0.03),2,5.09 (0.06),NGU22,1,,,NRAOVLA,+18 47 18.8782,-02 06 16.751,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.8286590,-2.1046530,30.5888740,-0.0427210,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G30.5887-0.0427, 1,5(-1)->6(0)_A+,G30.622+0.082,G30.6214+0.0826,,15.0000000000,281.7322570,-2.0183010,30.6217530,0.0824060,,,,39.98,,18.000,0.49 (0.01),2,0.45 (0.02),NGU22,1,,,NRAOVLA,+18 46 55.7417,-02 01 5.885,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.7322570,-2.0183010,30.6217530,0.0824060,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G30.6218+0.0824, 1,5(-1)->6(0)_A+,G30.702-0.068,G30.7028-0.0683,,15.0000000000,281.9033040,-2.0150810,30.7026140,-0.0682340,,,,88.3,,18.000,126.8 (1.08),2,122.44 (1.85),NGU22,1,,,NRAOVLA,+18 47 36.7929,-02 00 54.293,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.9033040,-2.0150810,30.7026140,-0.0682340,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G30.7025-0.0681, 1,5(-1)->6(0)_A+,G30.758-0.050,G30.7599-0.0523,,15.0000000000,281.9155330,-1.9568910,30.7599720,-0.0525620,,,,91.68,,18.000,43.12 (0.22),2,41.65 (0.38),NGU22,1,,,NRAOVLA,+18 47 39.7279,-01 57 24.806,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.9155330,-1.9568910,30.7599720,-0.0525620,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G30.7584-0.0497, 1,5(-1)->6(0)_A+,G30.770-0.804,G30.7700-0.8043,,15.0000000000,282.5898750,-2.2910880,30.7698570,-0.8046940,,,,75.9,,18.000,12.58 (0.07),2,12.51 (0.13),NGU22,1,,,NRAOVLA,+18 50 21.5701,-02 17 27.918,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,282.5898750,-2.2910880,30.7698570,-0.8046940,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G30.7703-0.8040, 1,5(-1)->6(0)_A+,G30.770-0.804,G30.7700-0.8043,,15.0000000000,282.5898770,-2.2910890,30.7698560,-0.8046960,,,,74.46,,18.000,8.08 (0.06),2,7.9 (0.1),NGU22,1,,,NRAOVLA,+18 50 21.5704,-02 17 27.922,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,282.5898770,-2.2910890,30.7698560,-0.8046960,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G30.7703-0.8040, 1,5(-1)->6(0)_A+,G30.774+0.078,G30.7744+0.0783,,15.0000000000,281.8057650,-1.8845020,30.7743340,0.0780880,,,,98.46,,18.000,0.99 (0.02),2,1.07 (0.04),NGU22,1,,,NRAOVLA,+18 47 13.3835,-01 53 4.207,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.8057650,-1.8845020,30.7743340,0.0780880,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G30.7744+0.0781, 1,5(-1)->6(0)_A+,G30.781+0.231,G30.7799+0.2301,,15.0000000000,281.6729440,-1.8102780,30.7798040,0.2300820,,,,48.97,,18.000,29.03 (0.27),2,27.44 (0.46),NGU22,1,,,NRAOVLA,+18 46 41.5065,-01 48 37.002,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.6729440,-1.8102780,30.7798040,0.2300820,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G30.7808+0.2306, 1,5(-1)->6(0)_A+,G30.788+0.204,G30.7880+0.2039,,15.0000000000,281.7003450,-1.8150160,30.7880860,0.2035500,,,,84.98,,18.000,17.04 (0.13),2,16.23 (0.22),NGU22,1,,,NRAOVLA,+18 46 48.0829,-01 48 54.059,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.7003450,-1.8150160,30.7880860,0.2035500,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G30.7881+0.2038, 1,5(-1)->6(0)_A+,G30.817-0.057,G30.8176-0.0547,,15.0000000000,281.9437870,-1.9066820,30.8175340,-0.0547850,,,,93.2,,18.000,4.87 (0.04),2,4.74 (0.06),NGU22,1,,,NRAOVLA,+18 47 46.5089,-01 54 24.055,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.9437870,-1.9066820,30.8175340,-0.0547850,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G30.8175-0.0569, 1,5(-1)->6(0)_A+,G30.817-0.057,G30.8178-0.0570,,15.0000000000,281.9457250,-1.9072990,30.8178680,-0.0567900,,,,109.03,,18.000,15.42 (0.08),2,15.07 (0.13),NGU22,1,,,NRAOVLA,+18 47 46.9739,-01 54 26.278,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.9457250,-1.9072990,30.8178680,-0.0567900,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G30.8175-0.0569, 1,5(-1)->6(0)_A+,G30.010-0.273,G30.0095-0.2734,,15.0000000000,281.7696500,-2.7253230,30.0096750,-0.2734540,,,,106.06,,18.000,2.36 (0.02),2,2.34 (0.03),NGU22,1,,,NRAOVLA,+18 47 4.716,-02 43 31.162,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.7696500,-2.7253230,30.0096750,-0.2734540,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G30.0097-0.2734, 1,5(-1)->6(0)_A+,G30.819+0.273,G30.8184+0.2725,,15.0000000000,281.6524600,-1.7562880,30.8185020,0.2729380,,,,100.35,,18.000,1.48 (0.03),2,1.6 (0.06),NGU22,1,,,NRAOVLA,+18 46 36.5903,-01 45 22.635,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.6524600,-1.7562880,30.8185020,0.2729380,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G30.8185+0.2734, 1,5(-1)->6(0)_A+,G30.860+0.124,G30.8507+0.1221,,15.0000000000,281.8011390,-1.7963430,30.8506720,0.1224270,,,,28.78,,18.000,0.95 (0.02),2,0.95 (0.03),NGU22,1,,,NRAOVLA,+18 47 12.2733,-01 47 46.834,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.8011390,-1.7963430,30.8506720,0.1224270,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G30.8507+0.1225, 1,5(-1)->6(0)_A+,G30.898+0.162,G30.8979+0.1612,,15.0000000000,281.7880270,-1.7369230,30.8975660,0.1612010,,,,101.84,,18.000,55.15 (0.27),2,53.62 (0.47),NGU22,1,,,NRAOVLA,+18 47 9.1264,-01 44 12.924,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.7880270,-1.7369230,30.8975660,0.1612010,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G30.8980+0.1615, 1,5(-1)->6(0)_A+,G30.959+0.086,G30.9584+0.0861,,15.0000000000,281.8830920,-1.7169260,30.9587150,0.0857690,,,,39.98,,18.000,0.45 (0.02),2,0.44 (0.03),NGU22,1,,,NRAOVLA,+18 47 31.9422,-01 43 0.934,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.8830920,-1.7169260,30.9587150,0.0857690,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G30.9588+0.0862, 1,5(-1)->6(0)_A+,G30.972-0.141,G30.9726-0.1414,,15.0000000000,282.0918030,-1.8084920,30.9723970,-0.1416430,,,,77.83,,18.000,21.71 (0.17),2,20.58 (0.29),NGU22,1,,,NRAOVLA,+18 48 22.0327,-01 48 30.573,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,282.0918030,-1.8084920,30.9723970,-0.1416430,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G30.9725-0.1416, 1,5(-1)->6(0)_A+,G30.980+0.216,G30.9801+0.2158,,15.0000000000,281.7770360,-1.6389360,30.9797460,0.2156860,,,,110.92,,18.000,0.7 (0.02),2,0.7 (0.04),NGU22,1,,,NRAOVLA,+18 47 6.4886,-01 38 20.169,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.7770360,-1.6389360,30.9797460,0.2156860,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G30.9796+0.2157, 1,5(-1)->6(0)_A+,G30.973+0.562,G30.9729+0.5624,,15.0000000000,281.4656030,-1.4869560,30.9729090,0.5620520,,,,19.88,,18.000,0.44 (0.02),2,0.41 (0.03),NGU22,1,,,NRAOVLA,+18 45 51.7448,-01 29 13.041,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.4656030,-1.4869560,30.9729090,0.5620520,0.018,,,,,0.18,1,D,,,G30.9728+0.5622, 1,5(-1)->6(0)_A+,G30.199-0.169,G30.1981-0.1688,,15.0000000000,281.7627650,-2.5100500,30.1980950,-0.1691080,,,,108.58,,18.000,18.43 (0.22),2,17.27 (0.36),NGU22,1,,,NRAOVLA,+18 47 3.0636,-02 30 36.179,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.7627650,-2.5100500,30.1980950,-0.1691080,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G30.1980-0.1690, 1,5(-1)->6(0)_A+,G30.199-0.169,G30.2244-0.1803,,15.0000000000,281.7845450,-2.4914720,30.2245540,-0.1799930,,,,113.03,,18.000,15.86 (0.13),2,14.76 (0.22),NGU22,1,,,NRAOVLA,+18 47 8.2908,-02 29 29.299,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.7845450,-2.4914720,30.2245540,-0.1799930,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G30.2245-0.1797, 1,5(-1)->6(0)_A+,G30.317+0.070,G30.3177+0.0703,,15.0000000000,281.6042630,-2.2947320,30.3174160,0.0700630,,,,36.42,,18.000,7.72 (0.05),2,7.44 (0.09),NGU22,1,,,NRAOVLA,+18 46 25.0231,-02 17 41.037,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.6042630,-2.2947320,30.3174160,0.0700630,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G30.3174+0.0701, 1,5(-1)->6(0)_A+,G30.370+0.482,G30.3705+0.4827,,15.0000000000,281.2613200,-2.0593530,30.3703990,0.4824170,,,,12.33,,18.000,6.32 (0.04),2,6.13 (0.06),NGU22,1,,,NRAOVLA,+18 45 2.7169,-02 03 33.672,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.2613200,-2.0593530,30.3703990,0.4824170,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G30.3703+0.4824, 1,5(-1)->6(0)_A+,G30.400-0.296,G30.4006-0.2958,,15.0000000000,281.9679050,-2.3877610,30.4004220,-0.2956950,,,,105.07,,18.000,4.85 (0.03),2,4.69 (0.05),NGU22,1,,,NRAOVLA,+18 47 52.2972,-02 23 15.939,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.9679050,-2.3877610,30.4004220,-0.2956950,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G30.4004-0.2958, 1,5(-1)->6(0)_A+,G30.419-0.232,G30.4194-0.2316,,15.0000000000,281.9198030,-2.3419250,30.4192860,-0.2320170,,,,102.96,,18.000,13.65 (0.11),2,13.06 (0.19),NGU22,1,,,NRAOVLA,+18 47 40.7527,-02 20 30.93,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.9198030,-2.3419250,30.4192860,-0.2320170,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G30.4194-0.2324, 1,5(-1)->6(0)_A+,G30.423+0.465,G30.4234+0.4661,,15.0000000000,281.3003110,-2.0196870,30.4234820,0.4658610,,,,5.9,,18.000,0.65 (0.02),2,0.63 (0.04),NGU22,1,,,NRAOVLA,+18 45 12.0747,-02 01 10.873,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.3003110,-2.0196870,30.4234820,0.4658610,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G30.4235+0.4655, 1,5(-1)->6(0)_A+,G30.536+0.019,G30.5426+0.0110,,15.0000000000,281.7593470,-2.1215010,30.5422780,0.0112260,,,,54.45,,18.000,0.6 (0.02),2,0.59 (0.03),NGU22,1,,,NRAOVLA,+18 47 2.2432,-02 07 17.402,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.7593470,-2.1215010,30.5422780,0.0112260,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G30.5422+0.0111, 1,5(-1)->6(0)_A+,G31.396-0.257,G31.3959-0.2576,,15.0000000000,282.3877460,-1.4843230,31.3958080,-0.2570600,,,,87.31,,18.000,0.38 (0.02),2,0.34 (0.03),NGU22,1,,,NRAOVLA,+18 49 33.0591,-01 29 3.562,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,282.3877460,-1.4843230,31.3958080,-0.2570600,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G31.3956-0.2569, 1,5(-1)->6(0)_A+,G31.412+0.307,G31.4122+0.3071,,15.0000000000,281.8929010,-1.2126040,31.4119700,0.3071260,,,,95.81,,18.000,14.59 (0.16),2,13.81 (0.27),NGU22,1,,,NRAOVLA,+18 47 34.2963,-01 12 45.375,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.8929010,-1.2126040,31.4119700,0.3071260,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G31.4117+0.3070, 1,5(-1)->6(0)_A+,G31.581+0.077,G31.5811+0.0769,,15.0000000000,282.1747880,-1.1673230,31.5808240,0.0769840,,,,98.82,,18.000,6.49 (0.07),2,6.12 (0.12),NGU22,1,,,NRAOVLA,+18 48 41.9492,-01 10 2.362,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,282.1747880,-1.1673230,31.5808240,0.0769840,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G31.5809+0.0770, 1,5(-1)->6(0)_A+,G31.594-0.192,G31.5937-0.1920,,15.0000000000,282.4204610,-1.2784850,31.5939120,-0.1922990,,,,48.25,,18.000,4.01 (0.03),2,3.83 (0.06),NGU22,1,,,NRAOVLA,+18 49 40.9106,-01 16 42.547,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,282.4204610,-1.2784850,31.5939120,-0.1922990,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G31.5937-0.1923, 1,5(-1)->6(0)_A+,G31.974+0.178,G31.9747+0.1803,,15.0000000000,282.2641590,-0.7708450,31.9744190,0.1782900,,,,92.62,,18.000,0.67 (0.12),2,1.25 (0.33),NGU22,1,,,NRAOVLA,+18 49 3.3981,-00 46 15.042,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,282.2641590,-0.7708450,31.9744190,0.1782900,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G31.9744+0.1783, 1,5(-1)->6(0)_A+,G31.047+0.356,G31.0470+0.3562,,15.0000000000,281.6827600,-1.5150810,31.0469550,0.3560580,,,,82.73,,18.000,4.37 (0.04),2,4.09 (0.07),NGU22,1,,,NRAOVLA,+18 46 43.8624,-01 30 54.291,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.6827600,-1.5150810,31.0469550,0.3560580,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G31.0472+0.3561, 1,5(-1)->6(0)_A+,G31.060+0.093,G31.0592+0.0933,,15.0000000000,281.9222310,-1.6240640,31.0591980,0.0933210,,,,16.51,,18.000,17.77 (0.12),2,17.09 (0.21),NGU22,1,,,NRAOVLA,+18 47 41.3355,-01 37 26.63,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.9222310,-1.6240640,31.0591980,0.0933210,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G31.0599+0.0933, 1,5(-1)->6(0)_A+,G31.078+0.459,G31.0767+0.4573,,15.0000000000,281.6059320,-1.4425550,31.0764420,0.4574940,,,,25.68,,18.000,2.07 (0.02),2,1.98 (0.04),NGU22,1,,,NRAOVLA,+18 46 25.4236,-01 26 33.197,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.6059320,-1.4425550,31.0764420,0.4574940,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G31.0776+0.4591, 1,5(-1)->6(0)_A+,G31.122+0.063,G31.1213+0.0628,,15.0000000000,281.9777290,-1.5825770,31.1214250,0.0628810,,,,48.07,,18.000,2.08 (0.02),2,1.99 (0.04),NGU22,1,,,NRAOVLA,+18 47 54.655,-01 34 57.276,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,281.9777290,-1.5825770,31.1214250,0.0628810,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G31.1216+0.0628, 1,5(-1)->6(0)_A+,G31.159+0.046,G31.1580+0.0457,,15.0000000000,282.0096800,-1.5575710,31.1582470,0.0458660,,,,41.14,,18.000,2.08 (0.03),2,2.01 (0.05),NGU22,1,,,NRAOVLA,+18 48 2.3231,-01 33 27.255,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,282.0096800,-1.5575710,31.1582470,0.0458660,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G31.1585+0.0456, 1,5(-1)->6(0)_A+,G31.182-0.148,G31.1824-0.1477,,15.0000000000,282.1933510,-1.6244090,31.1825130,-0.1480090,,,,46.31,,18.000,2.09 (0.02),2,2.05 (0.03),NGU22,1,,,NRAOVLA,+18 48 46.4042,-01 37 27.874,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,282.1933510,-1.6244090,31.1825130,-0.1480090,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G31.1825-0.1481, 1,5(-1)->6(0)_A+,G31.253+0.002,G31.2526+0.0029,,15.0000000000,282.0916090,-1.4934590,31.2526600,0.0022280,,,,41.14,,18.000,0.24 (0.01),2,0.24 (0.03),NGU22,1,,,NRAOVLA,+18 48 21.9862,-01 29 36.451,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,282.0916090,-1.4934590,31.2526600,0.0022280,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G31.2527+0.0025, 1,5(-1)->6(0)_A+,G31.276+0.005,G31.2756+0.0053,,15.0000000000,282.0995340,-1.4717770,31.2755680,0.0050680,,,,37.46,,18.000,0.4 (0.01),2,0.39 (0.02),NGU22,1,,,NRAOVLA,+18 48 23.8882,-01 28 18.399,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,282.0995340,-1.4717770,31.2755680,0.0050680,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G31.2756+0.0051, 1,5(-1)->6(0)_A+,G31.280+0.062,G31.2805+0.0617,,15.0000000000,282.0515570,-1.4418030,31.2803650,0.0614220,,,,110.29,,18.000,62.2 (0.69),2,58.05 (1.16),NGU22,1,,,NRAOVLA,+18 48 12.3736,-01 26 30.491,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,282.0515570,-1.4418030,31.2803650,0.0614220,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G31.2804+0.0618, 1,5(-1)->6(0)_A+,G32.914-0.096,G32.9175-0.0935,,15.0000000000,282.9362520,-0.0555380,32.9174960,-0.0936500,,,,103.45,,18.000,1.49 (0.01),2,1.45 (0.03),NGU22,1,,,NRAOVLA,+18 51 44.7005,-00 03 19.937,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,282.9362520,-0.0555380,32.9174960,-0.0936500,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G32.9175-0.0936, 1,5(-1)->6(0)_A+,G32.963-0.340,G32.9645-0.3394,,15.0000000000,283.1765890,-0.1259830,32.9643900,-0.3396690,,,,48.38,,18.000,0.54 (0.02),2,0.56 (0.03),NGU22,1,,,NRAOVLA,+18 52 42.3814,-00 07 33.539,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,283.1765890,-0.1259830,32.9643900,-0.3396690,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G32.9630-0.3400, 1,5(-1)->6(0)_A+,G32.993+0.038,G32.9918+0.0343,,15.0000000000,282.8565800,0.0685430,32.9915980,0.0338360,,,,91,,18.000,12.53 (0.07),2,12.14 (0.12),NGU22,1,,,NRAOVLA,+18 51 25.5793,+00 04 6.753,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,282.8565800,0.0685430,32.9915980,0.0338360,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G32.9924+0.0381, 1,5(-1)->6(0)_A+,G32.045+0.059,G32.0446+0.0593,,15.0000000000,282.4023410,-0.7627110,32.0446700,0.0590350,,,,92.62,,18.000,110.72 (0.86),2,108.66 (1.52),NGU22,1,,,NRAOVLA,+18 49 36.5618,-00 45 45.761,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,282.4023410,-0.7627110,32.0446700,0.0590350,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G32.0448+0.0589, 1,5(-1)->6(0)_A+,G32.102-0.075,G32.1056-0.0741,,15.0000000000,282.5485330,-0.7694800,32.1053070,-0.0741460,,,,49.87,,18.000,0.3 (0.02),2,0.31 (0.04),NGU22,1,,,NRAOVLA,+18 50 11.6478,-00 46 10.129,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,282.5485330,-0.7694800,32.1053070,-0.0741460,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G32.1024-0.0749, 1,5(-1)->6(0)_A+,G32.117+0.092,G32.1176+0.0906,,15.0000000000,282.4072370,-0.6834600,32.1174340,0.0908200,,,,92.71,,18.000,11.04 (0.16),2,10.24 (0.28),NGU22,1,,,NRAOVLA,+18 49 37.7369,-00 41 0.455,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,282.4072370,-0.6834600,32.1174340,0.0908200,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G32.1175+0.0908, 1,5(-1)->6(0)_A+,G32.516+0.323,G32.5150+0.3229,,15.0000000000,282.3821900,-0.2239490,32.5149640,0.3226610,,,,52.65,,18.000,1.27 (0.01),2,1.2 (0.02),NGU22,1,,,NRAOVLA,+18 49 31.7255,-00 13 26.215,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,282.3821900,-0.2239490,32.5149640,0.3226610,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G32.5163+0.3233, 1,5(-1)->6(0)_A+,G32.706-0.059,G32.7039-0.0555,,15.0000000000,282.8050700,-0.2287210,32.7035490,-0.0558670,,,,40.78,,18.000,0.15 (0.02),2,0.26 (0.04),NGU22,1,,,NRAOVLA,+18 51 13.2167,-00 13 43.394,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,282.8050700,-0.2287210,32.7035490,-0.0558670,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G32.7035-0.0559, 1,5(-1)->6(0)_A+,G32.744-0.076,G32.7443-0.0753,,15.0000000000,282.8410720,-0.2015520,32.7441450,-0.0755210,,,,38.49,,18.000,44.62 (0.31),2,42.51 (0.53),NGU22,1,,,NRAOVLA,+18 51 21.8573,-00 12 5.587,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,282.8410720,-0.2015520,32.7441450,-0.0755210,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G32.7440-0.0756, 1,5(-1)->6(0)_A+,G32.744-0.076,G32.7496-0.0642,,15.0000000000,282.8333460,-0.1916230,32.7494580,-0.0641170,,,,34.98,,18.000,2.73 (0.03),2,2.67 (0.05),NGU22,1,,,NRAOVLA,+18 51 20.003,-00 11 29.844,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,282.8333460,-0.1916230,32.7494580,-0.0641170,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G32.7495-0.0640, 1,5(-1)->6(0)_A+,G32.797+0.191,G32.8027+0.1926,,15.0000000000,282.6290980,-0.0275680,32.8023310,0.1924680,,,,26.89,,18.000,0.69 (0.02),2,0.64 (0.03),NGU22,1,,,NRAOVLA,+18 50 30.9834,-00 01 39.244,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,282.6290980,-0.0275680,32.8023310,0.1924680,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G32.8024+0.1925, 1,5(-1)->6(0)_A+,G32.827-0.316,G32.8212-0.3301,,15.0000000000,283.1029400,-0.2494070,32.8209600,-0.3304000,,,,82.23,,18.000,1.22 (0.02),2,1.13 (0.03),NGU22,1,,,NRAOVLA,+18 52 24.7057,-00 14 57.864,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,283.1029400,-0.2494070,32.8209600,-0.3304000,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G32.8213-0.3300, 1,5(-1)->6(0)_A+,G33.641-0.228,G33.6412-0.2276,,15.0000000000,283.3856550,0.5275200,33.6413350,-0.2277260,,,,60.3,,18.000,113.97 (0.29),2,112.62 (0.51),NGU22,1,,,NRAOVLA,+18 53 32.5572,+00 31 39.072,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,283.3856550,0.5275200,33.6413350,-0.2277260,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G33.6414-0.2277, 1,5(-1)->6(0)_A+,G33.726-0.120,G33.7258-0.1202,,15.0000000000,283.3282530,0.6513250,33.7253410,-0.1201830,,,,54.09,,18.000,4.41 (0.04),2,4.19 (0.06),NGU22,1,,,NRAOVLA,+18 53 18.7807,+00 39 4.771,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,283.3282530,0.6513250,33.7253410,-0.1201830,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G33.7254-0.1202, 1,5(-1)->6(0)_A+,G33.852+0.017,G33.8520+0.0178,,15.0000000000,283.2630580,0.8269760,33.8519340,0.0179360,,,,63.58,,18.000,8.33 (0.04),2,8.33 (0.07),NGU22,1,,,NRAOVLA,+18 53 3.1339,+00 49 37.112,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,283.2630580,0.8269760,33.8519340,0.0179360,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G33.8517+0.0179, 1,5(-1)->6(0)_A+,G33.980-0.019,G33.9798-0.0189,,15.0000000000,283.3542390,0.9238200,33.9796990,-0.0190370,,,,64.03,,18.000,1.95 (0.01),2,1.93 (0.02),NGU22,1,,,NRAOVLA,+18 53 25.0174,+00 55 25.752,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,283.3542390,0.9238200,33.9796990,-0.0190370,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G33.9798-0.0190, 1,5(-1)->6(0)_A+,G33.093-0.072,G33.0925-0.0725,,15.0000000000,282.9975020,0.1094210,33.0922370,-0.0729430,,,,104.22,,18.000,12.24 (0.06),2,11.72 (0.11),NGU22,1,,,NRAOVLA,+18 51 59.4005,+00 06 33.914,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,282.9975020,0.1094210,33.0922370,-0.0729430,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G33.0922-0.0729, 1,5(-1)->6(0)_A+,G33.133-0.092,G33.1328-0.0916,,15.0000000000,283.0325620,0.1367280,33.1325260,-0.0916940,,,,73.2,,18.000,13.3 (0.03),2,13.23 (0.06),NGU22,1,,,NRAOVLA,+18 52 7.8149,+00 08 12.219,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,283.0325620,0.1367280,33.1325260,-0.0916940,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G33.1326-0.0915, 1,5(-1)->6(0)_A+,G33.202-0.008,G33.1996+0.0010,,15.0000000000,282.9806340,0.2387680,33.1996630,0.0010500,,,,91.36,,18.000,0.67 (0.02),2,0.63 (0.03),NGU22,1,,,NRAOVLA,+18 51 55.3522,+00 14 19.566,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,282.9806340,0.2387680,33.1996630,0.0010500,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G33.1997+0.0010, 1,5(-1)->6(0)_A+,G33.202-0.008,G33.2037-0.0101,,15.0000000000,282.9921300,0.2372450,33.2035490,-0.0098750,,,,92.08,,18.000,0.89 (0.02),2,0.81 (0.03),NGU22,1,,,NRAOVLA,+18 51 58.1112,+00 14 14.083,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,282.9921300,0.2372450,33.2035490,-0.0098750,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G33.2017-0.0082, 1,5(-1)->6(0)_A+,G33.317-0.360,G33.3174-0.3599,,15.0000000000,283.3553810,0.1788420,33.3172140,-0.3597910,,,,29.14,,18.000,0.84 (0.01),2,0.81 (0.02),NGU22,1,,,NRAOVLA,+18 53 25.2915,+00 10 43.831,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,283.3553810,0.1788420,33.3172140,-0.3597910,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G33.3172-0.3598, 1,5(-1)->6(0)_A+,G33.393+0.010,G33.3930+0.0097,,15.0000000000,283.0610040,0.4145610,33.3927630,0.0096830,,,,105.12,,18.000,18.47 (0.07),2,18.24 (0.12),NGU22,1,,,NRAOVLA,+18 52 14.641,+00 24 52.419,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,283.0610040,0.4145610,33.3927630,0.0096830,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G33.3928+0.0097, 1,5(-1)->6(0)_A+,G33.425-0.315,G33.4246-0.3150,,15.0000000000,283.3643710,0.2948050,33.4245190,-0.3149100,,,,45.76,,18.000,0.28 (0.01),2,0.26 (0.03),NGU22,1,,,NRAOVLA,+18 53 27.449,+00 17 41.297,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,283.3643710,0.2948050,33.4245190,-0.3149100,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G33.4246-0.3149, 1,5(-1)->6(0)_A+,G33.486+0.040,G33.4870+0.0407,,15.0000000000,283.0766560,0.5125940,33.4871480,0.0404560,,,,120.49,,18.000,2.59 (0.02),2,2.57 (0.04),NGU22,1,,,NRAOVLA,+18 52 18.3975,+00 30 45.34,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,283.0766560,0.5125940,33.4871480,0.0404560,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G33.4859+0.0398, 1,5(-1)->6(0)_A+,G33.644-0.025,G33.6339-0.0206,,15.0000000000,283.1981890,0.6150860,33.6337790,-0.0209630,,,,103,,18.000,1.34 (0.02),2,1.28 (0.03),NGU22,1,,,NRAOVLA,+18 52 47.5653,+00 36 54.308,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,283.1981890,0.6150860,33.6337790,-0.0209630,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G33.6337-0.0210, 1,5(-1)->6(0)_A+,G34.757+0.024,G34.7567+0.0250,,15.0000000000,283.6697400,1.6351140,34.7565640,0.0246810,,,,76.48,,18.000,1.45 (0.02),2,1.47 (0.03),NGU22,1,,,NRAOVLA,+18 54 40.7377,+01 38 6.411,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,283.6697400,1.6351140,34.7565640,0.0246810,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G34.7566+0.0246, 1,5(-1)->6(0)_A+,G34.821+0.352,G34.8221+0.3518,,15.0000000000,283.4079990,1.8418580,34.8212280,0.3518010,,,,59.75,,18.000,0.14 (0.01),2,0.18 (0.03),NGU22,1,,,NRAOVLA,+18 53 37.9197,+01 50 30.69,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,283.4079990,1.8418580,34.8212280,0.3518010,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G34.8206+0.3518, 1,5(-1)->6(0)_A+,G34.096+0.016,G34.0957+0.0178,,15.0000000000,283.3745890,1.0440730,34.0959980,0.0176970,,,,55.93,,18.000,5.86 (0.03),2,5.74 (0.05),NGU22,1,,,NRAOVLA,+18 53 29.9013,+01 02 38.664,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,283.3745890,1.0440730,34.0959980,0.0176970,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G34.0960+0.0176, 1,5(-1)->6(0)_A+,G34.196-0.592,G34.1953-0.5928,,15.0000000000,283.9634950,0.8538960,34.1953430,-0.5930520,,,,61.78,,18.000,0.4 (0.01),2,0.43 (0.02),NGU22,1,,,NRAOVLA,+18 55 51.2389,+00 51 14.024,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,283.9634950,0.8538960,34.1953430,-0.5930520,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G34.1963-0.5919, 1,5(-1)->6(0)_A+,G34.257+0.153,G34.2448+0.1333,,15.0000000000,283.3393810,1.2294210,34.2448970,0.1335510,,,,61.15,,18.000,6.52 (0.04),2,6.34 (0.07),NGU22,1,,,NRAOVLA,+18 53 21.4515,+01 13 45.917,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,283.3393810,1.2294210,34.2448970,0.1335510,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G34.2443+0.1333, 1,5(-1)->6(0)_A+,G34.257+0.153,G34.2582+0.1534,,15.0000000000,283.3276740,1.2500720,34.2579370,0.1533850,,,,57.51,,18.000,23.39 (0.08),2,22.93 (0.13),NGU22,1,,,NRAOVLA,+18 53 18.6417,+01 15 0.258,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,283.3276740,1.2500720,34.2579370,0.1533850,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G34.2572+0.1532, 1,5(-1)->6(0)_A+,G34.267-0.210,G34.2672-0.2094,,15.0000000000,283.6552140,1.0926780,34.2672230,-0.2098280,,,,54.54,,18.000,9.64 (0.02),2,9.68 (0.04),NGU22,1,,,NRAOVLA,+18 54 37.2513,+01 05 33.642,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,283.6552140,1.0926780,34.2672230,-0.2098280,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G34.2672-0.2098, 1,5(-1)->6(0)_A+,G34.283+0.183,G34.2839+0.1837,,15.0000000000,283.3127630,1.2867660,34.2837950,0.1833860,,,,52.02,,18.000,0.26 (0.02),2,0.35 (0.04),NGU22,1,,,NRAOVLA,+18 53 15.063,+01 17 12.358,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,283.3127630,1.2867660,34.2837950,0.1833860,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G34.2833+0.1834, 1,5(-1)->6(0)_A+,G34.403+0.232,G34.3957+0.2215,,15.0000000000,283.3295460,1.4038410,34.3956410,0.2218430,,,,55.71,,18.000,15.84 (0.04),2,15.74 (0.07),NGU22,1,,,NRAOVLA,+18 53 19.0911,+01 24 13.829,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,283.3295460,1.4038410,34.3956410,0.2218430,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G34.3940+0.2214, 1,5(-1)->6(0)_A+,G34.403+0.232,G34.4113+0.2349,,15.0000000000,283.3250330,1.4237550,34.4113060,0.2349390,,,,63.44,,18.000,0.53 (0.02),2,0.57 (0.03),NGU22,1,,,NRAOVLA,+18 53 18.008,+01 25 25.517,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,283.3250330,1.4237550,34.4113060,0.2349390,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G34.4112+0.2350, 1,5(-1)->6(0)_A+,G34.751-0.093,G34.7510-0.0925,,15.0000000000,283.7717480,1.5767420,34.7511340,-0.0926870,,,,53.06,,18.000,5.41 (0.01),2,5.42 (0.03),NGU22,1,,,NRAOVLA,+18 55 5.2196,+01 34 36.27,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,283.7717480,1.5767420,34.7511340,-0.0926870,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G34.7511-0.0927, 1,5(-1)->6(0)_A+,G35.575+0.067,G35.5879+0.0605,,15.0000000000,284.0175100,2.3911050,35.5878550,0.0603240,,,,43.98,,18.000,0.3 (0.02),2,0.29 (0.03),NGU22,1,,,NRAOVLA,+18 56 4.2024,+02 23 27.979,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,284.0175100,2.3911050,35.5878550,0.0603240,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G35.5880+0.0603, 1,5(-1)->6(0)_A+,G35.793-0.175,G35.7927-0.1744,,15.0000000000,284.3203270,2.4661190,35.7926920,-0.1746280,,,,60.75,,18.000,25.58 (0.1),2,25.44 (0.17),NGU22,1,,,NRAOVLA,+18 57 16.8784,+02 27 58.028,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,284.3203270,2.4661190,35.7926920,-0.1746280,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G35.7927-0.1747, 1,5(-1)->6(0)_A+,G35.025+0.350,G35.0248+0.3497,,15.0000000000,283.5027500,2.0219540,35.0246950,0.3496560,,,,44.38,,18.000,19.49 (0.05),2,19.64 (0.08),NGU22,1,,,NRAOVLA,+18 54 0.66,+02 01 19.034,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,283.5027500,2.0219540,35.0246950,0.3496560,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G35.0247+0.3497, 1,5(-1)->6(0)_A+,G35.131-0.746,G35.1327-0.7440,,15.0000000000,284.5255040,1.6187450,35.1323860,-0.7439380,,,,31.16,,18.000,11.15 (0.06),2,11.25 (0.1),NGU22,1,,,NRAOVLA,+18 58 6.121,+01 37 7.481,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,284.5255040,1.6187450,35.1323860,-0.7439380,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G35.1313-0.7458, 1,5(-1)->6(0)_A+,G35.149+0.808,G35.1491+0.8095,,15.0000000000,283.1500410,2.3420840,35.1489180,0.8093040,,,,72.02,,18.000,1.22 (0.02),2,1.28 (0.04),NGU22,1,,,NRAOVLA,+18 52 36.0098,+02 20 31.503,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,283.1500410,2.3420840,35.1489180,0.8093040,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G35.1488+0.8077, 1,5(-1)->6(0)_A+,G35.197-0.743,G35.1973-0.7428,,15.0000000000,284.5543470,1.6765980,35.1970250,-0.7431730,,,,28.51,,18.000,157.12 (0.45),2,157.1 (0.79),NGU22,1,,,NRAOVLA,+18 58 13.0432,+01 40 35.752,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,284.5543470,1.6765980,35.1970250,-0.7431730,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G35.1966-0.7428, 1,5(-1)->6(0)_A+,G35.228-0.358,G35.2260-0.3544,,15.0000000000,284.2218050,1.8797410,35.2260270,-0.3547100,,,,59.49,,18.000,0.38 (0.02),2,0.39 (0.04),NGU22,1,,,NRAOVLA,+18 56 53.2332,+01 52 47.068,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,284.2218050,1.8797410,35.2260270,-0.3547100,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G35.2260-0.3547, 1,5(-1)->6(0)_A+,G35.247-0.237,G35.2476-0.2365,,15.0000000000,284.1266320,1.9524070,35.2472680,-0.2369100,,,,72.25,,18.000,1.4 (0.02),2,1.47 (0.03),NGU22,1,,,NRAOVLA,+18 56 30.3917,+01 57 8.664,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,284.1266320,1.9524070,35.2472680,-0.2369100,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G35.2473-0.2369, 1,5(-1)->6(0)_A+,G35.397+0.025,G35.3974+0.0252,,15.0000000000,283.9616140,2.2051940,35.3969420,0.0251860,,,,89.07,,18.000,0.36 (0.01),2,0.36 (0.02),NGU22,1,,,NRAOVLA,+18 55 50.7873,+02 12 18.699,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,283.9616140,2.2051940,35.3969420,0.0251860,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G35.3971+0.0253, 1,5(-1)->6(0)_A+,G35.417-0.284,G35.4166-0.2839,,15.0000000000,284.2460570,2.0817950,35.4168700,-0.2840460,,,,56.11,,18.000,1.67 (0.02),2,1.69 (0.03),NGU22,1,,,NRAOVLA,+18 56 59.0536,+02 04 54.463,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,284.2460570,2.0817950,35.4168700,-0.2840460,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G35.4169-0.2840, 1,5(-1)->6(0)_A+,G35.457-0.179,G35.4571-0.1782,,15.0000000000,284.1708970,2.1659480,35.4574610,-0.1788070,,,,56.11,,18.000,0.26 (0.02),2,0.31 (0.05),NGU22,1,,,NRAOVLA,+18 56 41.0152,+02 09 57.411,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,284.1708970,2.1659480,35.4574610,-0.1788070,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G35.4572-0.1790, 1,5(-1)->6(0)_A+,G36.115+0.554,G36.1152+0.5527,,15.0000000000,283.8197310,3.0848570,36.1150670,0.5526410,,,,72.65,,18.000,19.07 (0.08),2,18.91 (0.15),NGU22,1,,,NRAOVLA,+18 55 16.7355,+03 05 5.485,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,283.8197310,3.0848570,36.1150670,0.5526410,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G36.1151+0.5527, 1,5(-1)->6(0)_A+,G36.705+0.096,G36.7055+0.0964,,15.0000000000,284.4962990,3.4016470,36.7052430,0.0962000,,,,53,,18.000,2.28 (0.02),2,2.24 (0.04),NGU22,1,,,NRAOVLA,+18 57 59.1118,+03 24 5.928,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,284.4962990,3.4016470,36.7052430,0.0962000,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G36.7053+0.0962, 1,5(-1)->6(0)_A+,G36.839-0.022,G36.8395-0.0224,,15.0000000000,284.6633950,3.4669000,36.8394780,-0.0223730,,,,57.05,,18.000,3.29 (0.03),2,3.31 (0.06),NGU22,1,,,NRAOVLA,+18 58 39.2148,+03 28 0.839,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,284.6633950,3.4669000,36.8394780,-0.0223730,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G36.8395-0.0224, 1,5(-1)->6(0)_A+,G36.918+0.483,G36.9180+0.4825,,15.0000000000,284.2492270,3.7677820,36.9184100,0.4827530,,,,-36.05,,18.000,1.01 (0.02),2,0.93 (0.03),NGU22,1,,,NRAOVLA,+18 56 59.8144,+03 46 4.015,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,284.2492270,3.7677820,36.9184100,0.4827530,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G36.9183+0.4828, 1,5(-1)->6(0)_A+,G36.634-0.203,G36.6338-0.2030,,15.0000000000,284.7301930,3.2013560,36.6337340,-0.2030110,,,,77.4,,18.000,1.37 (0.03),2,1.48 (0.05),NGU22,1,,,NRAOVLA,+18 58 55.2463,+03 12 4.881,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,284.7301930,3.2013560,36.6337340,-0.2030110,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G36.6337-0.2030, 1,5(-1)->6(0)_A+,G37.735-0.112,G37.7349-0.1120,,15.0000000000,285.1535030,4.2220950,37.7346830,-0.1121030,,,,50.3,,18.000,0.93 (0.02),2,0.93 (0.04),NGU22,1,,,NRAOVLA,+19 00 36.8407,+04 13 19.541,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,285.1535030,4.2220950,37.7346830,-0.1121030,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G37.7348-0.1120, 1,5(-1)->6(0)_A+,G37.763-0.214,G37.7535-0.1892,,15.0000000000,285.2309820,4.2032730,37.7532900,-0.1894250,,,,60.56,,18.000,2.03 (0.03),2,2 (0.05),NGU22,1,,,NRAOVLA,+19 00 55.4358,+04 12 11.782,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,285.2309820,4.2032730,37.7532900,-0.1894250,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G37.7535-0.1893, 1,5(-1)->6(0)_A+,G37.763-0.214,G37.7676-0.2140,,15.0000000000,285.2594430,4.2043680,37.7672490,-0.2141640,,,,69.72,,18.000,0.4 (0.03),2,0.34 (0.04),NGU22,1,,,NRAOVLA,+19 01 2.2664,+04 12 15.724,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,285.2594430,4.2043680,37.7672490,-0.2141640,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G37.7672-0.2151, 1,5(-1)->6(0)_A+,G37.868-0.601,G37.8684-0.6002,,15.0000000000,285.6501110,4.1169560,37.8678790,-0.6006000,,,,51.1,,18.000,0.51 (0.02),2,0.54 (0.04),NGU22,1,,,NRAOVLA,+19 02 36.0266,+04 07 1.042,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,285.6501110,4.1169560,37.8678790,-0.6006000,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G37.8677-0.6012, 1,5(-1)->6(0)_A+,G37.038-0.035,G37.0425-0.0361,,15.0000000000,284.7684130,3.6423480,37.0434330,-0.0354490,,,,80.17,,18.000,12.22 (0.07),2,12.15 (0.13),NGU22,1,,,NRAOVLA,+18 59 4.4192,+03 38 32.451,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,284.7684130,3.6423480,37.0434330,-0.0354490,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G37.0435-0.0354, 1,5(-1)->6(0)_A+,G37.479-0.105,G37.4793-0.1048,,15.0000000000,285.0297440,3.9979190,37.4788710,-0.1048400,,,,62.05,,18.000,8.31 (0.07),2,8.2 (0.12),NGU22,1,,,NRAOVLA,+19 00 7.1386,+03 59 52.509,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,285.0297440,3.9979190,37.4788710,-0.1048400,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G37.4790-0.1048, 1,5(-1)->6(0)_A+,G37.546-0.112,G37.5460-0.1118,,15.0000000000,285.0666100,4.0545000,37.5460060,-0.1116740,,,,52.48,,18.000,4.63 (0.08),2,4.69 (0.14),NGU22,1,,,NRAOVLA,+19 00 15.9863,+04 03 16.201,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,285.0666100,4.0545000,37.5460060,-0.1116740,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G37.5460-0.1119, 1,5(-1)->6(0)_A+,G37.554+0.201,G37.5536+0.2007,,15.0000000000,284.7916140,4.2040490,37.5536380,0.2006350,,,,83.67,,18.000,6.04 (0.04),2,5.98 (0.08),NGU22,1,,,NRAOVLA,+18 59 9.9874,+04 12 14.576,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,284.7916140,4.2040490,37.5536380,0.2006350,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G37.5538+0.2008, 1,5(-1)->6(0)_A+,G37.598+0.425,G37.5981+0.4250,,15.0000000000,284.6116830,4.3459970,37.5979340,0.4250960,,,,87.18,,18.000,17.12 (0.15),2,16.89 (0.25),NGU22,1,,,NRAOVLA,+18 58 26.804,+04 20 45.59,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,284.6116830,4.3459970,37.5979340,0.4250960,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G37.5979+0.4251, 1,5(-1)->6(0)_A+,G37.193+0.032,G37.1932+0.0320,,15.0000000000,284.7765280,3.8065480,37.1931890,0.0323800,,,,86.1,,18.000,0.29 (0.02),2,0.29 (0.04),NGU22,1,,,NRAOVLA,+18 59 6.3668,+03 48 23.574,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,284.7765280,3.8065480,37.1931890,0.0323800,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G37.1930+0.0323, 1,5(-1)->6(0)_A+,G37.038-0.035,G37.0303-0.0386,,15.0000000000,284.7651530,3.6291590,37.0302150,-0.0385810,,,,78.32,,18.000,2.51 (0.03),2,2.46 (0.05),NGU22,1,,,NRAOVLA,+18 59 3.6367,+03 37 44.971,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,284.7651530,3.6291590,37.0302150,-0.0385810,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G37.0303-0.0386, 1,5(-1)->6(0)_A+,G38.565+0.538,G38.5655+0.5378,,15.0000000000,284.9547280,5.2579300,38.5653340,0.5376910,,,,-28.8,,18.000,1.19 (0.03),2,1.17 (0.04),NGU22,1,,,NRAOVLA,+18 59 49.1347,+05 15 28.548,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,284.9547280,5.2579300,38.5653340,0.5376910,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G38.5654+0.5378, 1,5(-1)->6(0)_A+,G38.598-0.213,G38.5978-0.2126,,15.0000000000,285.6393970,4.9430220,38.5973470,-0.2127810,,,,63.84,,18.000,0.29 (0.02),2,0.28 (0.03),NGU22,1,,,NRAOVLA,+19 02 33.4552,+04 56 34.878,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,285.6393970,4.9430220,38.5973470,-0.2127810,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G38.5977-0.2126, 1,5(-1)->6(0)_A+,G38.038-0.300,G38.0371-0.3008,,15.0000000000,285.4601750,4.4050050,38.0372480,-0.3003250,,,,55.66,,18.000,6.18 (0.04),2,6.3 (0.07),NGU22,1,,,NRAOVLA,+19 01 50.4419,+04 24 18.019,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,285.4601750,4.4050050,38.0372480,-0.3003250,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G38.0375-0.3003, 1,5(-1)->6(0)_A+,G38.119-0.229,G38.1190-0.2293,,15.0000000000,285.4338900,4.5103920,38.1189520,-0.2287880,,,,70.28,,18.000,7.82 (0.09),2,7.86 (0.16),NGU22,1,,,NRAOVLA,+19 01 44.1336,+04 30 37.411,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,285.4338900,4.5103920,38.1189520,-0.2287880,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G38.1190-0.2288, 1,5(-1)->6(0)_A+,G38.203-0.067,G38.2037-0.0668,,15.0000000000,285.3279810,4.6595400,38.2032500,-0.0666640,,,,79.76,,18.000,10 (0.06),2,10.05 (0.11),NGU22,1,,,NRAOVLA,+19 01 18.7154,+04 39 34.345,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,285.3279810,4.6595400,38.2032500,-0.0666640,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G38.2033-0.0667, 1,5(-1)->6(0)_A+,G38.255-0.200,G38.2551-0.2001,,15.0000000000,285.4706710,4.6443570,38.2548410,-0.2000630,,,,69.42,,18.000,1.13 (0.02),2,1.06 (0.03),NGU22,1,,,NRAOVLA,+19 01 52.961,+04 38 39.684,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,285.4706710,4.6443570,38.2548410,-0.2000630,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G38.2548-0.2001, 1,5(-1)->6(0)_A+,G38.258-0.074,G38.2579-0.0737,,15.0000000000,285.3591660,4.7049640,38.2578610,-0.0735130,,,,15.29,,18.000,9.1 (0.05),2,9.07 (0.09),NGU22,1,,,NRAOVLA,+19 01 26.1998,+04 42 17.869,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,285.3591660,4.7049640,38.2578610,-0.0735130,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G38.2578-0.0737, 1,5(-1)->6(0)_A+,G38.653+0.088,G38.6531+0.0874,,15.0000000000,285.3968420,5.1297980,38.6527730,0.0875400,,,,-31.42,,18.000,1.81 (0.02),2,1.84 (0.03),NGU22,1,,,NRAOVLA,+19 01 35.2421,+05 07 47.273,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,285.3968420,5.1297980,38.6527730,0.0875400,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G38.6528+0.0875, 1,5(-1)->6(0)_A+,G38.917-0.353,G38.9163-0.3529,,15.0000000000,285.9110470,5.1618970,38.9158850,-0.3530080,,,,32.33,,18.000,0.79 (0.03),2,0.81 (0.05),NGU22,1,,,NRAOVLA,+19 03 38.6512,+05 09 42.828,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,285.9110470,5.1618970,38.9158850,-0.3530080,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G38.9158-0.3531, 1,5(-1)->6(0)_A+,G38.578-0.549,G38.5774-0.5494,,15.0000000000,285.9304940,4.7712940,38.5776080,-0.5492790,,,,70.64,,18.000,0.43 (0.02),2,0.46 (0.04),NGU22,1,,,NRAOVLA,+19 03 43.3185,+04 46 16.657,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,285.9304940,4.7712940,38.5776080,-0.5492790,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G38.5776-0.5493, 1,5(-1)->6(0)_A+,G38.076-0.266,G38.0764-0.2653,,15.0000000000,285.4469200,4.4557890,38.0763500,-0.2653300,,,,67.5,,18.000,0.43 (0.02),2,0.43 (0.03),NGU22,1,,,NRAOVLA,+19 01 47.2607,+04 27 20.841,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,285.4469200,4.4557890,38.0763500,-0.2653300,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G38.0765-0.2655, 1,5(-1)->6(0)_A+,G39.100+0.491,G39.1005+0.4918,,15.0000000000,285.2417250,5.7126090,39.1003470,0.4915190,,,,15.74,,18.000,22.98 (0.43),2,22.92 (0.75),NGU22,1,,,NRAOVLA,+19 00 58.0139,+05 42 45.394,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,285.2417250,5.7126090,39.1003470,0.4915190,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G39.1002+0.4912, 1,5(-1)->6(0)_A+,G39.388-0.141,G39.3881-0.1409,,15.0000000000,285.9388540,5.6786510,39.3878330,-0.1407070,,,,60.34,,18.000,0.55 (0.02),2,0.55 (0.03),NGU22,1,,,NRAOVLA,+19 03 45.325,+05 40 43.145,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,285.9388540,5.6786510,39.3878330,-0.1407070,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G39.3877-0.1406, 1,5(-1)->6(0)_A+,G39.536-0.382,G39.5364-0.3782,,15.0000000000,286.2191360,5.7023440,39.5368180,-0.3776690,,,,48.16,,18.000,0.13 (0.02),2,0.15 (0.03),NGU22,1,,,NRAOVLA,+19 04 52.5926,+05 42 8.437,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,286.2191360,5.7023440,39.5368180,-0.3776690,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G39.5367-0.3777, 1,5(-1)->6(0)_A+,G40.282-0.220,G40.2819-0.2195,,15.0000000000,286.4216850,6.4368490,40.2818170,-0.2193760,,,,74.32,,18.000,28.68 (0.12),2,28.33 (0.2),NGU22,1,,,NRAOVLA,+19 05 41.2043,+06 26 12.658,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,286.4216850,6.4368490,40.2818170,-0.2193760,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G40.2819-0.2195, 1,5(-1)->6(0)_A+,G40.425+0.700,G40.4250+0.6999,,15.0000000000,285.6649520,6.9858940,40.4250310,0.7002760,,,,15.47,,18.000,21.63 (0.2),2,21.51 (0.35),NGU22,1,,,NRAOVLA,+19 02 39.5885,+06 59 9.217,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,285.6649520,6.9858940,40.4250310,0.7002760,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G40.4250+0.7001, 1,5(-1)->6(0)_A+,G40.597-0.718,G40.5965-0.7189,,15.0000000000,287.0136380,6.4868340,40.5966920,-0.7187060,,,,76.08,,18.000,1.32 (0.02),2,1.29 (0.04),NGU22,1,,,NRAOVLA,+19 08 3.2731,+06 29 12.601,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,287.0136380,6.4868340,40.5966920,-0.7187060,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G40.5973-0.7185, 1,5(-1)->6(0)_A+,G40.623-0.138,G40.6222-0.1383,,15.0000000000,286.5067550,6.7767650,40.6225640,-0.1382800,,,,31.12,,18.000,12.16 (0.1),2,11.94 (0.18),NGU22,1,,,NRAOVLA,+19 06 1.6212,+06 46 36.354,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,286.5067550,6.7767650,40.6225640,-0.1382800,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G40.6225-0.1383, 1,5(-1)->6(0)_A+,G40.934-0.041,G40.9340-0.0411,,15.0000000000,286.5640100,7.0983330,40.9342860,-0.0409870,,,,36.56,,18.000,2.12 (0.03),2,2.12 (0.04),NGU22,1,,,NRAOVLA,+19 06 15.3625,+07 05 53.998,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,286.5640100,7.0983330,40.9342860,-0.0409870,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G40.9344-0.0410, 1,5(-1)->6(0)_A+,G41.509-0.105,G41.5086-0.1054,,15.0000000000,286.8878080,7.5789980,41.5087990,-0.1050850,,,,64.21,,18.000,0.75 (0.02),2,0.75 (0.03),NGU22,1,,,NRAOVLA,+19 07 33.074,+07 34 44.394,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,286.8878080,7.5789980,41.5087990,-0.1050850,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G41.5088-0.1051, 1,5(-1)->6(0)_A+,G41.050-0.247,G41.0505-0.2476,,15.0000000000,286.8021880,7.1063330,41.0500710,-0.2471900,,,,65.36,,18.000,0.15 (0.02),2,0.32 (0.05),NGU22,1,,,NRAOVLA,+19 07 12.5252,+07 06 22.799,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,286.8021880,7.1063330,41.0500710,-0.2471900,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G41.0495-0.2470, 1,5(-1)->6(0)_A+,G41.075-0.125,G41.0755-0.1247,,15.0000000000,286.7042690,7.1852480,41.0754520,-0.1246210,,,,56.16,,18.000,0.2 (0.02),2,0.22 (0.03),NGU22,1,,,NRAOVLA,+19 06 49.0245,+07 11 6.891,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,286.7042690,7.1852480,41.0754520,-0.1246210,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G41.0754-0.1247, 1,5(-1)->6(0)_A+,G41.577+0.041,G41.5760+0.0399,,15.0000000000,286.7882030,7.7069650,41.5769880,0.0414460,,,,11.72,,18.000,0.45 (0.02),2,0.51 (0.03),NGU22,1,,,NRAOVLA,+19 07 9.1687,+07 42 25.073,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,286.7882030,7.7069650,41.5769880,0.0414460,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G41.5770+0.0414, 1,5(-1)->6(0)_A+,G41.121-0.107,G41.1211-0.1068,,15.0000000000,286.7091830,7.2337020,41.1207220,-0.1066680,,,,37.14,,18.000,1.07 (0.02),2,1.06 (0.04),NGU22,1,,,NRAOVLA,+19 06 50.204,+07 14 1.327,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,286.7091830,7.2337020,41.1207220,-0.1066680,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G41.1208-0.1068, 1,5(-1)->6(0)_A+,G41.123-0.220,G41.1232-0.2200,,15.0000000000,286.8118690,7.1834590,41.1229690,-0.2202350,,,,63.31,,18.000,2.61 (0.03),2,2.55 (0.04),NGU22,1,,,NRAOVLA,+19 07 14.8485,+07 11 0.451,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,286.8118690,7.1834590,41.1229690,-0.2202350,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G41.1230-0.2202, 1,5(-1)->6(0)_A+,G41.156-0.201,G41.1538-0.2013,,15.0000000000,286.8098580,7.2215910,41.1559080,-0.2009200,,,,55.93,,18.000,5.41 (0.04),2,5.26 (0.07),NGU22,1,,,NRAOVLA,+19 07 14.366,+07 13 17.727,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,286.8098580,7.2215910,41.1559080,-0.2009200,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G41.1560-0.2009, 1,5(-1)->6(0)_A+,G41.226-0.197,G41.2260-0.1971,,15.0000000000,286.8390630,7.2855090,41.2259890,-0.1972330,,,,57.15,,18.000,5.91 (0.04),2,5.81 (0.08),NGU22,1,,,NRAOVLA,+19 07 21.375,+07 17 7.833,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,286.8390630,7.2855090,41.2259890,-0.1972330,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G41.2261-0.1972, 1,5(-1)->6(0)_A+,G41.226-0.197,G41.2294-0.2084,,15.0000000000,286.8504790,7.2828730,41.2288590,-0.2085000,,,,57.15,,18.000,0.33 (0),2,0.38 (0.01),NGU22,1,,,NRAOVLA,+19 07 24.1149,+07 16 58.344,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,286.8504790,7.2828730,41.2288590,-0.2085000,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G41.2289-0.2085, 1,5(-1)->6(0)_A+,G41.307-0.169,G41.3073-0.1688,,15.0000000000,286.8513580,7.3701100,41.3067130,-0.1691310,,,,51.03,,18.000,0.37 (0.02),2,0.38 (0.04),NGU22,1,,,NRAOVLA,+19 07 24.3258,+07 22 12.396,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,286.8513580,7.3701100,41.3067130,-0.1691310,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G41.3068-0.1692, 1,5(-1)->6(0)_A+,G41.268+0.372,G41.2683+0.3723,,15.0000000000,286.3482120,7.5845280,41.2678260,0.3724690,,,,20.29,,18.000,0.31 (0.03),2,0.31 (0.05),NGU22,1,,,NRAOVLA,+19 05 23.571,+07 35 4.301,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,286.3482120,7.5845280,41.2678260,0.3724690,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G41.2681+0.3725, 1,5(-1)->6(0)_A+,G41.348-0.136,G41.3475-0.1367,,15.0000000000,286.8409950,7.4213640,41.3474890,-0.1364230,,,,11.7,,18.000,17.61 (0.11),2,17.23 (0.2),NGU22,1,,,NRAOVLA,+19 07 21.8389,+07 25 16.909,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,286.8409950,7.4213640,41.3474890,-0.1364230,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G41.3476-0.1364, 1,5(-1)->6(0)_A+,G41.651+0.997,G41.6510+0.9967,,15.0000000000,285.9657410,8.2114630,41.6511560,0.9966890,,,,-42.56,,18.000,0.45 (0.02),2,0.39 (0.03),NGU22,1,,,NRAOVLA,+19 03 51.7778,+08 12 41.268,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,285.9657410,8.2114630,41.6511560,0.9966890,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G41.6512+0.9967, 1,5(-1)->6(0)_A+,G42.034+0.190,G42.0344+0.1902,,15.0000000000,286.8672620,8.1814830,42.0343200,0.1902620,,,,12.91,,18.000,20.69 (0.08),2,20.23 (0.14),NGU22,1,,,NRAOVLA,+19 07 28.143,+08 10 53.339,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,286.8672620,8.1814830,42.0343200,0.1902620,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G42.0344+0.1901, 1,5(-1)->6(0)_A+,G42.304-0.299,G42.3038-0.2994,,15.0000000000,287.4316830,8.1950610,42.3038160,-0.2992930,,,,28.02,,18.000,3.93 (0.03),2,3.91 (0.06),NGU22,1,,,NRAOVLA,+19 09 43.6038,+08 11 42.22,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,287.4316830,8.1950610,42.3038160,-0.2992930,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G42.3036-0.2994, 1,5(-1)->6(0)_A+,G42.435-0.260,G42.4351-0.2605,,15.0000000000,287.4577690,8.3292950,42.4348170,-0.2602490,,,,66.64,,18.000,1.95 (0.02),2,1.98 (0.04),NGU22,1,,,NRAOVLA,+19 09 49.8645,+08 19 45.463,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,287.4577690,8.3292950,42.4348170,-0.2602490,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G42.4348-0.2604, 1,5(-1)->6(0)_A+,G42.698-0.147,G42.6983-0.1473,,15.0000000000,287.4794250,8.6149460,42.6981100,-0.1474100,,,,-42.92,,18.000,3.83 (0.04),2,3.85 (0.08),NGU22,1,,,NRAOVLA,+19 09 55.0621,+08 36 53.804,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,287.4794250,8.6149460,42.6981100,-0.1474100,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G42.6981-0.1475, 1,5(-1)->6(0)_A+,G43.167+0.011,G43.1707+0.0043,,15.0000000000,287.5639750,9.1041830,43.1706540,0.0043580,,,,18.94,,18.000,13.04 (0.02),2,12.91 (0.04),NGU22,1,,,NRAOVLA,+19 10 15.3541,+09 06 15.057,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,287.5639750,9.1041830,43.1706540,0.0043580,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G43.1668+0.0106, 1,5(-1)->6(0)_A+,G43.167+0.011,G43.1749-0.0158,,15.0000000000,287.5838150,9.0987010,43.1748390,-0.0155490,,,,10.53,,18.000,0.35 (0.02),2,0.28 (0.03),NGU22,1,,,NRAOVLA,+19 10 20.1156,+09 05 55.324,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,287.5838150,9.0987010,43.1748390,-0.0155490,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G43.1749-0.0153, 1,5(-1)->6(0)_A+,G43.179-0.519,G43.1798-0.5186,,15.0000000000,288.0375670,8.8705880,43.1798120,-0.5184210,,,,64.97,,18.000,2.73 (0.02),2,2.74 (0.04),NGU22,1,,,NRAOVLA,+19 12 9.0161,+08 52 14.116,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,288.0375670,8.8705880,43.1798120,-0.5184210,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G43.1789-0.5186, 1,5(-1)->6(0)_A+,G43.795-0.127,G43.7958-0.1270,,15.0000000000,287.9749350,9.5973990,43.7954630,-0.1271880,,,,40.2,,18.000,24.9 (0.12),2,24.58 (0.21),NGU22,1,,,NRAOVLA,+19 11 53.9843,+09 35 50.636,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,287.9749350,9.5973990,43.7954630,-0.1271880,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G43.7955-0.1272, 1,5(-1)->6(0)_A+,G43.890-0.784,G43.8902-0.7846,,15.0000000000,288.6101490,9.3767270,43.8904370,-0.7846160,,,,47.93,,18.000,10.67 (0.08),2,10.7 (0.15),NGU22,1,,,NRAOVLA,+19 14 26.4358,+09 22 36.219,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,288.6101490,9.3767270,43.8904370,-0.7846160,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G43.8900-0.7844, 1,5(-1)->6(0)_A+,G43.525+0.017,G43.5302+0.0171,,15.0000000000,287.7205800,9.4292410,43.5303490,0.0174520,,,,51.96,,18.000,0.12 (0.01),2,0.13 (0.03),NGU22,1,,,NRAOVLA,+19 10 52.9391,+09 25 45.266,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,287.7205800,9.4292410,43.5303490,0.0174520,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G43.5302+0.0174, 1,5(-1)->6(0)_A+,G43.079+0.003,G43.0886-0.0113,,15.0000000000,287.5395220,9.0234650,43.0879070,-0.0114950,,,,14.46,,18.000,0.13 (0.02),2,0.21 (0.04),NGU22,1,,,NRAOVLA,+19 10 9.4854,+09 01 24.474,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,287.5395220,9.0234650,43.0879070,-0.0114950,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G43.0882-0.0114, 1,5(-1)->6(0)_A+,G43.038-0.453,G43.0381-0.4527,,15.0000000000,287.9124040,8.7750540,43.0378810,-0.4529900,,,,54.77,,18.000,5.72 (0.04),2,5.74 (0.07),NGU22,1,,,NRAOVLA,+19 11 38.9769,+08 46 30.193,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,287.9124040,8.7750540,43.0378810,-0.4529900,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G43.0383-0.4530, 1,5(-1)->6(0)_A+,G43.074-0.077,G43.0742-0.0770,,15.0000000000,287.5918570,8.9809490,43.0740660,-0.0769770,,,,10.17,,18.000,7.07 (0.06),2,7 (0.11),NGU22,1,,,NRAOVLA,+19 10 22.0457,+08 58 51.417,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,287.5918570,8.9809490,43.0740660,-0.0769770,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G43.0741-0.0770, 1,5(-1)->6(0)_A+,G43.061-0.003,G43.0605-0.0025,,15.0000000000,287.5187810,9.0032640,43.0605300,-0.0026510,,,,15.75,,18.000,1.98 (0.03),2,2.02 (0.05),NGU22,1,,,NRAOVLA,+19 10 4.5075,+09 00 11.751,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,287.5187810,9.0032640,43.0605300,-0.0026510,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G43.0605-0.0027, 1,5(-1)->6(0)_A+,G43.167+0.011,G43.1492+0.0133,,15.0000000000,287.5460470,9.0889280,43.1489490,0.0130170,,,,13.32,,18.000,15.13 (0.08),2,15 (0.13),NGU22,1,,,NRAOVLA,+19 10 11.0512,+09 05 20.142,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,287.5460470,9.0889280,43.1489490,0.0130170,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G43.1490+0.0131, 1,5(-1)->6(0)_A+,G43.167+0.011,G43.1708+0.0107,,15.0000000000,287.5584190,9.1064160,43.1701020,0.0102560,,,,13.68,,18.000,3.06 (0.07),2,2.84 (0.12),NGU22,1,,,NRAOVLA,+19 10 14.0206,+09 06 23.099,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,287.5584190,9.1064160,43.1701020,0.0102560,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G43.1668+0.0106, 1,5(-1)->6(0)_A+,G43.167+0.011,G43.1761+0.0154,,15.0000000000,287.5565400,9.1138200,43.1758130,0.0153210,,,,22.14,,18.000,0.56 (0.03),2,0.55 (0.05),NGU22,1,,,NRAOVLA,+19 10 13.5696,+09 06 49.753,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,287.5565400,9.1138200,43.1758130,0.0153210,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G43.1758+0.0153, 1,5(-1)->6(0)_A+,G43.167+0.011,G43.1652+0.0126,,15.0000000000,287.5536660,9.1033100,43.1651800,0.0129850,,,,9.31,,18.000,35.61 (0.14),2,35.25 (0.25),NGU22,1,,,NRAOVLA,+19 10 12.8798,+09 06 11.917,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,287.5536660,9.1033100,43.1651800,0.0129850,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G43.1668+0.0106, 1,5(-1)->6(0)_A+,G43.167+0.011,G43.1693+0.0158,,15.0000000000,287.5532000,9.1075320,43.1687120,0.0153430,,,,6.97,,18.000,0.76 (0.03),2,0.85 (0.05),NGU22,1,,,NRAOVLA,+19 10 12.7679,+09 06 27.114,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,287.5532000,9.1075320,43.1687120,0.0153430,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G43.1687+0.0153, 1,5(-1)->6(0)_A+,G43.167+0.011,G43.1673-0.0040,,15.0000000000,287.5696330,9.0974200,43.1672360,-0.0037200,,,,-1.25,,18.000,1.71 (0.03),2,1.75 (0.05),NGU22,1,,,NRAOVLA,+19 10 16.7119,+09 05 50.712,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,287.5696330,9.0974200,43.1672360,-0.0037200,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G43.1674-0.0037, 1,5(-1)->6(0)_A+,G44.310+0.041,G44.3105+0.0402,,15.0000000000,288.0658310,10.1313400,44.3101980,0.0406260,,,,56.02,,18.000,0.35 (0.02),2,0.37 (0.03),NGU22,1,,,NRAOVLA,+19 12 15.7995,+10 07 52.825,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,288.0658310,10.1313400,44.3101980,0.0406260,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G44.3104+0.0407, 1,5(-1)->6(0)_A+,G44.290+0.033,G44.2896+0.0314,,15.0000000000,288.0648070,10.1088360,44.2897850,0.0310990,,,,46.84,,18.000,0.3 (0.02),2,0.27 (0.03),NGU22,1,,,NRAOVLA,+19 12 15.5537,+10 06 31.81,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,288.0648070,10.1088360,44.2897850,0.0310990,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G44.2903+0.0327, 1,5(-1)->6(0)_A+,G44.644-0.516,G44.6438-0.5161,,15.0000000000,288.7240930,10.1687430,44.6439770,-0.5160110,,,,49.19,,18.000,0.64 (0.02),2,0.63 (0.04),NGU22,1,,,NRAOVLA,+19 14 53.7824,+10 10 7.473,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,288.7240930,10.1687430,44.6439770,-0.5160110,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G44.6440-0.5159, 1,5(-1)->6(0)_A+,G45.071+0.132,G45.0712+0.1321,,15.0000000000,288.3422710,10.8480080,45.0712280,0.1319080,,,,57.69,,18.000,45.66 (0.2),2,45.38 (0.34),NGU22,1,,,NRAOVLA,+19 13 22.145,+10 50 52.83,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,288.3422710,10.8480080,45.0712280,0.1319080,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G45.0712+0.1323, 1,5(-1)->6(0)_A+,G45.380-0.594,G45.3795-0.5936,,15.0000000000,289.1422020,10.7837110,45.3796750,-0.5935940,,,,53.46,,18.000,2.41 (0.02),2,2.37 (0.03),NGU22,1,,,NRAOVLA,+19 16 34.1284,+10 47 1.359,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,289.1422020,10.7837110,45.3796750,-0.5935940,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G45.3798-0.5936, 1,5(-1)->6(0)_A+,G45.465+0.053,G45.4448+0.0682,,15.0000000000,288.5762210,11.1497210,45.4450690,0.0685440,,,,49.96,,18.000,1.13 (0.01),2,1.17 (0.03),NGU22,1,,,NRAOVLA,+19 14 18.2931,+11 08 58.997,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,288.5762210,11.1497210,45.4450690,0.0685440,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G45.4451+0.0685, 1,5(-1)->6(0)_A+,G45.465+0.053,G45.4549+0.0596,,15.0000000000,288.5886070,11.1543150,45.4547810,0.0599170,,,,51.58,,18.000,0.15 (0.02),2,0.16 (0.03),NGU22,1,,,NRAOVLA,+19 14 21.2657,+11 09 15.534,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,288.5886070,11.1543150,45.4547810,0.0599170,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G45.4545+0.0596, 1,5(-1)->6(0)_A+,G45.465+0.053,G45.4670+0.0529,,15.0000000000,288.6006760,11.1620430,45.4671250,0.0530220,,,,56.61,,18.000,4.75 (0.02),2,4.68 (0.04),NGU22,1,,,NRAOVLA,+19 14 24.1622,+11 09 43.353,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,288.6006760,11.1620430,45.4671250,0.0530220,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G45.4671+0.0531, 1,5(-1)->6(0)_A+,G45.476+0.130,G45.4726+0.1335,,15.0000000000,288.5306990,11.2043670,45.4727210,0.1334740,,,,66.28,,18.000,4.87 (0.02),2,4.88 (0.03),NGU22,1,,,NRAOVLA,+19 14 7.3677,+11 12 15.722,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,288.5306990,11.2043670,45.4727210,0.1334740,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G45.4728+0.1335, 1,5(-1)->6(0)_A+,G45.476+0.130,G45.4927+0.1251,,15.0000000000,288.5473110,11.2183560,45.4926770,0.1255400,,,,57.15,,18.000,7 (0.02),2,6.91 (0.04),NGU22,1,,,NRAOVLA,+19 14 11.3546,+11 13 6.081,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,288.5473110,11.2183560,45.4926770,0.1255400,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G45.4927+0.1256, 1,5(-1)->6(0)_A+,G45.804-0.356,G45.8038-0.3561,,15.0000000000,289.1294050,11.2699720,45.8040220,-0.3557920,,,,59.94,,18.000,14.1 (0.08),2,13.85 (0.14),NGU22,1,,,NRAOVLA,+19 16 31.0572,+11 16 11.901,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,289.1294050,11.2699720,45.8040220,-0.3557920,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G45.8041-0.3559, 1,5(-1)->6(0)_A+,G45.568-0.120,G45.5706-0.1190,,15.0000000000,288.8043680,11.1707370,45.5677270,-0.1198640,,,,1.42,,18.000,0.29 (0.02),2,0.25 (0.02),NGU22,1,,,NRAOVLA,+19 15 13.0483,+11 10 14.655,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,288.8043680,11.1707370,45.5677270,-0.1198640,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G45.5684-0.1200, 1,5(-1)->6(0)_A+,G46.066+0.220,G46.0664+0.2201,,15.0000000000,288.7338240,11.7702390,46.0662880,0.2201650,,,,23.39,,18.000,1.04 (0.02),2,0.96 (0.04),NGU22,1,,,NRAOVLA,+19 14 56.1177,+11 46 12.86,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,288.7338240,11.7702390,46.0662880,0.2201650,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G46.0662+0.2203, 1,5(-1)->6(0)_A+,G46.115+0.387,G46.1150+0.3853,,15.0000000000,288.6062560,11.8905480,46.1147820,0.3866340,,,,58.54,,18.000,2.43 (0.02),2,2.51 (0.04),NGU22,1,,,NRAOVLA,+19 14 25.5015,+11 53 25.971,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,288.6062560,11.8905480,46.1147820,0.3866340,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G46.1148+0.3866, 1,5(-1)->6(0)_A+,G48.990-0.299,G48.9906-0.2987,,15.0000000000,290.6089790,14.1112010,48.9903460,-0.2988400,,,,71.62,,18.000,0.61 (0.03),2,0.56 (0.05),NGU22,1,,,NRAOVLA,+19 22 26.1549,+14 06 40.324,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,290.6089790,14.1112010,48.9903460,-0.2988400,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G48.9902-0.2991, 1,5(-1)->6(0)_A+,G48.902-0.273,G48.9023-0.2734,,15.0000000000,290.5431910,14.0455960,48.9024070,-0.2734860,,,,71.9,,18.000,0.33 (0.02),2,0.41 (0.03),NGU22,1,,,NRAOVLA,+19 22 10.3659,+14 02 44.147,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,290.5431910,14.0455960,48.9024070,-0.2734860,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G48.9022-0.2734, 1,5(-1)->6(0)_A+,G49.599-0.250,G49.5995-0.2495,,15.0000000000,290.8609500,14.6713250,49.5993560,-0.2496340,,,,62.28,,18.000,28.23 (0.13),2,28.39 (0.23),NGU22,1,,,NRAOVLA,+19 23 26.6279,+14 40 16.771,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,290.8609500,14.6713250,49.5993560,-0.2496340,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G49.5994-0.2495, 1,5(-1)->6(0)_A+,G49.543-0.883,G49.5428-0.8828,,15.0000000000,291.4094940,14.3218450,49.5430380,-0.8828870,,,,39.6,,18.000,1.67 (0.02),2,1.68 (0.04),NGU22,1,,,NRAOVLA,+19 25 38.2786,+14 19 18.641,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,291.4094940,14.3218450,49.5430380,-0.8828870,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G49.5430-0.8829, 1,5(-1)->6(0)_A+,G49.265+0.311,G49.2653+0.3112,,15.0000000000,290.1870600,14.6408190,49.2652540,0.3110460,,,,-5.14,,18.000,8.8 (0.04),2,8.84 (0.08),NGU22,1,,,NRAOVLA,+19 20 44.8945,+14 38 26.95,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,290.1870600,14.6408190,49.2652540,0.3110460,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G49.2652+0.3112, 1,5(-1)->6(0)_A+,G49.349+0.413,G49.3493+0.4126,,15.0000000000,290.1353160,14.7626600,49.3493030,0.4124670,,,,67.92,,18.000,8.83 (0.04),2,8.78 (0.07),NGU22,1,,,NRAOVLA,+19 20 32.4759,+14 45 45.575,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,290.1353160,14.7626600,49.3493030,0.4124670,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G49.3492+0.4125, 1,5(-1)->6(0)_A+,G49.416+0.326,G49.4157+0.3258,,15.0000000000,290.2466190,14.7804520,49.4155810,0.3258250,,,,-12,,18.000,6.9 (0.04),2,6.74 (0.07),NGU22,1,,,NRAOVLA,+19 20 59.1885,+14 46 49.629,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,290.2466190,14.7804520,49.4155810,0.3258250,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G49.4156+0.3257, 1,5(-1)->6(0)_A+,G49.416+0.326,G49.4167+0.3236,,15.0000000000,290.2491910,14.7802890,49.4166060,0.3235520,,,,-26.68,,18.000,2.43 (0.03),2,2.5 (0.05),NGU22,1,,,NRAOVLA,+19 20 59.8059,+14 46 49.042,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,290.2491910,14.7802890,49.4166060,0.3235520,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G49.4156+0.3257, 1,5(-1)->6(0)_A+,G49.488-0.387,G49.4698-0.3707,,15.0000000000,290.9079920,14.4996380,49.4695630,-0.3708920,,,,64.62,,18.000,3.24 (0.16),2,4.06 (0.33),NGU22,1,,,NRAOVLA,+19 23 37.918,+14 29 58.695,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,290.9079920,14.4996380,49.4695630,-0.3708920,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G49.4708-0.3709, 1,5(-1)->6(0)_A+,G50.315+0.676,G50.3149+0.6763,,15.0000000000,290.3644780,15.7383920,50.3144880,0.6759780,,,,30.04,,18.000,2.75 (0.03),2,2.66 (0.05),NGU22,1,,,NRAOVLA,+19 21 27.4748,+15 44 18.213,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,290.3644780,15.7383920,50.3144880,0.6759780,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G50.3146+0.6760, 1,5(-1)->6(0)_A+,G50.071+0.558,G50.0710+0.5575,,15.0000000000,290.3537800,15.4675880,50.0706620,0.5576700,,,,-7.77,,18.000,0.85 (0.01),2,0.82 (0.02),NGU22,1,,,NRAOVLA,+19 21 24.9073,+15 28 3.317,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,290.3537800,15.4675880,50.0706620,0.5576700,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G50.0708+0.5581, 1,5(-1)->6(0)_A+,G50.011+0.525,G50.0100+0.5246,,15.0000000000,290.3547080,15.3989990,50.0105550,0.5246130,,,,-5.25,,18.000,0.16 (0.02),2,0.21 (0.04),NGU22,1,,,NRAOVLA,+19 21 25.1299,+15 23 56.397,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,290.3547080,15.3989990,50.0105550,0.5246130,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G50.0106+0.5246, 1,5(-1)->6(0)_A+,G50.779+0.152,G50.7788+0.1520,,15.0000000000,291.0725510,15.9003720,50.7787980,0.1517890,,,,48.83,,18.000,2.77 (0.02),2,2.74 (0.04),NGU22,1,,,NRAOVLA,+19 24 17.4123,+15 54 1.339,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,291.0725510,15.9003720,50.7787980,0.1517890,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G50.7789+0.1518, 1,5(-1)->6(0)_A+,G51.677+0.719,G51.6787+0.7193,,15.0000000000,290.9952630,16.9614330,51.6785200,0.7191520,,,,7.16,,18.000,1.05 (0.02),2,1.14 (0.04),NGU22,1,,,NRAOVLA,+19 23 58.8631,+16 57 41.16,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,290.9952630,16.9614330,51.6785200,0.7191520,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G51.6774+0.7188, 1,5(-1)->6(0)_A+,G52.199+0.723,G52.1988+0.7229,,15.0000000000,291.2493320,17.4215240,52.1987330,0.7231950,,,,3.25,,18.000,5.15 (0.03),2,5.22 (0.06),NGU22,1,,,NRAOVLA,+19 24 59.8396,+17 25 17.488,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,291.2493320,17.4215240,52.1987330,0.7231950,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G52.1989+0.7232, 1,5(-1)->6(0)_A+,G52.922+0.414,G52.9217+0.4138,,15.0000000000,291.8958060,17.9103960,52.9217110,0.4136970,,,,39.44,,18.000,4.89 (0.06),2,4.87 (0.1),NGU22,1,,,NRAOVLA,+19 27 34.9935,+17 54 37.424,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,291.8958060,17.9103960,52.9217110,0.4136970,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G52.9218+0.4139, 1,5(-1)->6(0)_A+,G53.036+0.113,G53.0366+0.1129,,15.0000000000,292.2313130,17.8674700,53.0365140,0.1126880,,,,10.02,,18.000,1.54 (0.03),2,1.56 (0.05),NGU22,1,,,NRAOVLA,+19 28 55.515,+17 52 2.892,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,292.2313130,17.8674700,53.0365140,0.1126880,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G53.0365+0.1119, 1,5(-1)->6(0)_A+,G53.142+0.070,G53.1420+0.0705,,15.0000000000,292.3233280,17.9396240,53.1417770,0.0703490,,,,24.6,,18.000,0.63 (0.02),2,0.68 (0.04),NGU22,1,,,NRAOVLA,+19 29 17.5987,+17 56 22.645,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,292.3233280,17.9396240,53.1417770,0.0703490,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G53.1419+0.0704, 1,5(-1)->6(0)_A+,G53.618+0.035,G53.6181+0.0354,,15.0000000000,292.5959520,18.3406330,53.6179060,0.0353030,,,,18.82,,18.000,1.35 (0.02),2,1.37 (0.03),NGU22,1,,,NRAOVLA,+19 30 23.0285,+18 20 26.278,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,292.5959520,18.3406330,53.6179060,0.0353030,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G53.6180+0.0354, 1,5(-1)->6(0)_A+,G53.484+0.521,G53.4847+0.5209,,15.0000000000,292.0786670,18.4562720,53.4843350,0.5215740,,,,54.38,,18.000,0.18 (0.02),2,0.18 (0.04),NGU22,1,,,NRAOVLA,+19 28 18.88,+18 27 22.579,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,292.0786670,18.4562720,53.4843350,0.5215740,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G53.4843+0.5209, 1,5(-1)->6(0)_A+,G54.373-0.614,G54.3712-0.6133,,15.0000000000,293.5782220,18.6871960,54.3709470,-0.6132500,,,,37.68,,18.000,0.79 (0.03),2,0.8 (0.05),NGU22,1,,,NRAOVLA,+19 34 18.7733,+18 41 13.907,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,293.5782220,18.6871960,54.3709470,-0.6132500,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G54.3730-0.6140, 1,5(-1)->6(0)_A+,G56.962-0.234,G56.9634-0.2346,,15.0000000000,294.5712540,21.1348100,56.9631210,-0.2345830,,,,29.68,,18.000,1.92 (0.03),2,1.95 (0.05),NGU22,1,,,NRAOVLA,+19 38 17.101,+21 08 5.315,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,294.5712540,21.1348100,56.9631210,-0.2345830,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G56.9618-0.2340, 1,5(-1)->6(0)_A+,G57.610+0.025,G57.6104+0.0249,,15.0000000000,294.6697190,21.8257080,57.6100710,0.0246350,,,,31.96,,18.000,9.09 (0.06),2,9.18 (0.1),NGU22,1,,,NRAOVLA,+19 38 40.7325,+21 49 32.549,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,294.6697190,21.8257080,57.6100710,0.0246350,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G57.6101+0.0247, 1,5(-1)->6(0)_A+,G58.773+0.647,G58.7749+0.6437,,15.0000000000,294.7046950,23.1445240,58.7748020,0.6441360,,,,33.13,,18.000,7.04 (0.02),2,7.04 (0.04),NGU22,1,,,NRAOVLA,+19 38 49.1268,+23 08 40.288,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,294.7046950,23.1445240,58.7748020,0.6441360,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G58.7748+0.6452, 1,5(-1)->6(0)_A+,G58.098+0.744,G58.0983+0.7430,,15.0000000000,294.2512000,22.6032930,58.0982310,0.7432940,,,,46.68,,18.000,0.4 (0.02),2,0.46 (0.05),NGU22,1,,,NRAOVLA,+19 37 0.2879,+22 36 11.855,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,294.2512000,22.6032930,58.0982310,0.7432940,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G58.0980+0.7435, 1,5(-1)->6(0)_A+,G58.697+0.632,G58.6963+0.6315,,15.0000000000,294.6750200,23.0706430,58.6970340,0.6316350,,,,33.68,,18.000,1.12 (0.01),2,1.15 (0.03),NGU22,1,,,NRAOVLA,+19 38 42.0047,+23 04 14.315,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,294.6750200,23.0706430,58.6970340,0.6316350,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G58.6970+0.6316, 1,5(-1)->6(0)_A+,G59.833+0.671,G59.8333+0.6722,,15.0000000000,295.2470200,24.0789450,59.8328340,0.6720710,,,,38.21,,18.000,18.4 (0.41),2,21.21 (0.79),NGU22,1,,,NRAOVLA,+19 40 59.2847,+24 04 44.202,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,295.2470200,24.0789450,59.8328340,0.6720710,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G59.8326+0.6714, 1,5(-1)->6(0)_A+,G59.783+0.064,G59.7825+0.0645,,15.0000000000,295.7968390,23.7342390,59.7827830,0.0646410,,,,26.97,,18.000,40.57 (1.33),2,48.77 (2.65),NGU22,1,,,NRAOVLA,+19 43 11.2413,+23 44 3.262,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,295.7968390,23.7342390,59.7827830,0.0646410,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G59.7828+0.0640, 1,5(-1)->6(0)_A+,G59.634-0.189,G59.6332-0.1917,,15.0000000000,295.9581560,23.4768200,59.6332000,-0.1917570,,,,29.58,,18.000,2.79 (0.09),2,3.41 (0.18),NGU22,1,,,NRAOVLA,+19 43 49.9574,+23 28 36.553,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,295.9581560,23.4768200,59.6332000,-0.1917570,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G59.6335-0.1916, 1,5(-1)->6(0)_A+,G59.498-0.236,G59.4988-0.2367,,15.0000000000,295.9266060,23.3363730,59.4970130,-0.2366700,,,,27.85,,18.000,0.11 (0.02),2,0.24 (0.05),NGU22,1,,,NRAOVLA,+19 43 42.3855,+23 20 10.942,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,295.9266060,23.3363730,59.4970130,-0.2366700,0.018,Spectra of 6.7 GHz methanol masers detected with GLOSTAR extracted at the peak pixel. The red dashed line indicates the ATLASGAL clump velocity (Urquhart et al. 2018, 2022) in case of an associated 870 m compact source catalog (CSC) source.,,,,0.18,1,D,,,G59.4977-0.2362, 1,5(-1)->6(0)_A+,G76.092+0.141,G76.0932+0.1580,,15.0000000000,305.8486790,37.5933810,76.0930810,0.1579560,,,,0.54,,18.000,0.02 (0.55),2,0.03,NGU22,1,,,NRAOVLA,+20 23 23.683,+37 35 36.17,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,305.8486790,37.5933810,76.0930810,0.1579560,0.018,,,,,0.18,1,D,,,G76.0926+0.1577, 1,5(-1)->6(0)_A+,G76.844+0.123,G76.8437+0.1233,,15.0000000000,306.4323250,38.1870170,76.8436520,0.1232720,,,,4.61,,18.000,0.04 (4.7),2,0.08,NGU22,1,,,NRAOVLA,+20 25 43.758,+38 11 13.26,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,306.4323250,38.1870170,76.8436520,0.1232720,0.018,,,,,0.18,1,D,,,G76.8436+0.1232, 1,5(-1)->6(0)_A+,G78.887+0.709,G78.8870+0.7087,,15.0000000000,307.3539460,40.1888360,78.8869270,0.7086510,,,,0.77,,18.000,0.02 (0.8),2,0.04,NGU22,1,,,NRAOVLA,+20 29 24.947,+40 11 19.81,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,307.3539460,40.1888360,78.8869270,0.7086510,0.018,,,,,0.18,1,D,,,G78.8867+0.7089, 1,5(-1)->6(0)_A+,G78.969+0.541,G78.9690+0.5410,,15.0000000000,307.5946880,40.1566390,78.9689670,0.5408860,,,,1.16,,18.000,0.03 (1.22),2,0.06,NGU22,1,,,NRAOVLA,+20 30 22.725,+40 09 23.9,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,307.5946880,40.1566390,78.9689670,0.5408860,0.018,,,,,0.18,1,D,,,G78.9689+0.5409, 1,5(-1)->6(0)_A+,G78.988+0.221,G78.9884+0.2211,,15.0000000000,307.9470250,39.9834780,78.9883470,0.2210290,,,,1.87,,18.000,0.03 (1.97),2,0.06,NGU22,1,,,NRAOVLA,+20 31 47.286,+39 59 0.52,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,307.9470250,39.9834780,78.9883470,0.2210290,0.018,,,,,0.18,1,D,,,G78.9883+0.2210, 1,5(-1)->6(0)_A+,G79.736+0.990,G79.7358+0.9904,,15.0000000000,307.7112460,41.0409530,79.7357270,0.9903640,,,,23.21,,18.000,0.1 (23.42),2,0.17,NGU22,1,,,NRAOVLA,+20 30 50.699,+41 02 27.43,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,307.7112460,41.0409530,79.7357270,0.9903640,0.018,,,,,0.18,1,D,,,G79.7357+0.9901, 1,5(-1)->6(0)_A+,G80.861+0.383,G80.8617+0.3834,,15.0000000000,309.2541290,41.5822720,80.8616450,0.3833020,,,,11.79,,18.000,0.07 (11.89),2,0.12,NGU22,1,,,NRAOVLA,+20 37 0.991,+41 34 56.18,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,309.2541290,41.5822720,80.8616450,0.3833020,0.018,,,,,0.18,1,D,,,G80.8615+0.3834, 1,5(-1)->6(0)_A+,G81.711+0.563,G81.6788+0.5377,,15.0000000000,309.7548000,42.3257330,81.6787100,0.5376120,,,,-0.73,,18.000,0.03 (0.97),2,0.06,NGU22,1,,,NRAOVLA,+20 39 1.152,+42 19 32.64,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,309.7548000,42.3257330,81.6787100,0.5376120,0.018,,,,,0.18,1,D,,,G81.6757+0.5399, 1,5(-1)->6(0)_A+,G81.711+0.563,G81.7219+0.5711,,15.0000000000,309.7544420,42.3802470,81.7218220,0.5709790,,,,5.11,,18.000,0.04 (5.09),2,0.06,NGU22,1,,,NRAOVLA,+20 39 1.066,+42 22 48.89,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,309.7544420,42.3802470,81.7218220,0.5709790,0.018,,,,,0.18,1,D,,,G81.7216+0.5722, 1,5(-1)->6(0)_A+,G81.767+0.596,G81.7444+0.5910,,15.0000000000,309.7515370,42.4102780,81.7443570,0.5909470,,,,11.72,,18.000,0.21 (12.32),2,0.39,NGU22,1,,,NRAOVLA,+20 39 0.369,+42 24 37,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,309.7515370,42.4102780,81.7443570,0.5909470,0.018,,,,,0.18,1,D,,,G81.7444+0.5909, 1,5(-1)->6(0)_A+,G81.767+0.596,G81.7523+0.5908,,15.0000000000,309.7583170,42.4164250,81.7522810,0.5907130,,,,14.06,,18.000,0.07 (14.37),2,0.13,NGU22,1,,,NRAOVLA,+20 39 1.996,+42 24 59.13,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,309.7583170,42.4164250,81.7522810,0.5907130,0.018,,,,,0.18,1,D,,,G81.7523+0.5907, 1,5(-1)->6(0)_A+,G81.767+0.596,G81.7655+0.5972,,15.0000000000,309.7622710,42.4308140,81.7654780,0.5971480,,,,3.18,,18.000,0.17 (3.82),2,0.33,NGU22,1,,,NRAOVLA,+20 39 2.945,+42 25 50.93,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,309.7622710,42.4308140,81.7654780,0.5971480,0.018,,,,,0.18,1,D,,,G81.7670+0.5961, 1,5(-1)->6(0)_A+,G81.876+0.782,G81.8713+0.7807,,15.0000000000,309.6518130,42.6263060,81.8712550,0.7806040,,,,336.19,,18.000,1.65 (334.63),2,2.89,NGU22,1,,,NRAOVLA,+20 38 36.435,+42 37 34.7,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,309.6518130,42.6263060,81.8712550,0.7806040,0.018,,,,,0.18,1,D,,,G81.8775+0.7820, 1,5(-1)->6(0)_A+,G82.308+0.729,G82.3079+0.7296,,15.0000000000,310.0693420,42.9414220,82.3078620,0.7295450,,,,20.67,,18.000,0.07 (20.78),2,0.13,NGU22,1,,,NRAOVLA,+20 40 16.642,+42 56 29.12,Dec 2011 - Apr 2017,0,0,1,,,0,0,,,310.0693420,42.9414220,82.3078620,0.7295450,0.018,,,,,0.18,1,D,,,G82.3079+0.7293,

Software error:

can't write : No such file or directory at /var/www/html/download.pl line 400.

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