detected,source_name,other_name,ra,dec,l,b,vlow,vup,vpeak,vrange,rms,peak,int,ref,telescope_ref,units,ra_hms,dec_dms,class,grp,gc_flag,beam,gaia,date_txt,fwhm,line,rms_mjy_flag,mjy_flag,is_interf,dist,thermal,atlasgal,peak_num,rms_num,interf_l,interf_b,interf_ra,interf_dec,image2,image_descr,dist_parallax_num,dist_parallax,v_step,date_e,telescope_conf,rms_approx_flag,radec_interf,grpv,peak_num_all, ,,,deg. (J2000),deg. (J2000),(deg.),(deg.),(km/s),(km/s),(km/s),(km/s),(Jy),(Jy),(Jy*km/s),,,,(J2000),(J2000),,,,(arcsec),,,(km/s),,,,,(kpc),line mark,,,,,,,,,,,(kpc),(km/s),,,,,,, 1,U Her,,246.4456920,18.8922610,35.3439970,40.3526630,,,-18,-23;-12,,340,1370 (72),MEL93,JCMT,Jy,16 25 47,+18 53 32.1,,G35.345+40.351,0,16.000000000,,1992 March 28 - April 1,,7(53)->6(60),0,0,0,,0,,340.000,,35.3439970,40.3526630,246.4456920,18.8922610,,,,,1.1,,,1,(4.30128875275585 , 0.329732157596116),G35.3451+40.3509,340.000, 1,U Her,,0.6406910,0.2784090,97.7422010,-60.1810240,,,-17,-22;-11,,286,1430 (80),MEL93,JCMT,Jy,00 02 33.8,+00 16 42.3,,G97.742-60.181,0,16.000000000,,1992 March 28 - April 1,,6(43)->5(50),0,0,0,,0,,286.000,,97.7422010,-60.1810240,0.6406910,0.2784090,,,,,1.1,,,1,(0.011182167437895 , 0.00485915371718489),G97.7422-60.1810,286.000, 1,U Her,,0.6406910,0.2784090,97.7422010,-60.1810240,,,-16,-20;-10,,69,337 (36),MEL93,JCMT,Jy,00 02 33.8,+00 16 42.3,,G97.742-60.181,0,16.000000000,,1992 March 28 - April 1,,6(42)->5(51),0,0,0,,0,,69.000,,97.7422010,-60.1810240,0.6406910,0.2784090,,,,,1.1,,,1,(0.011182167437895 , 0.00485915371718489),G97.7422-60.1810,69.000, 1,G343-02,,283.3283270,1.2499100,34.2580910,0.1527300,,,59,46;68,,64,690 (40),MEL93,JCMT,Jy,18 53 18.8,+01 14 59.7,,G34.257+0.153,0,16.000000000,,1992 March 28 - April 1,,5(15)->4(22),0,0,0,,0,,64.000,,34.2580910,0.1527300,283.3283270,1.2499100,,Spectra of the 325,439, and 471 GHz H2O transitions (top to bottom) observed toward the star-forming regions G34.3-0.2, W49 N, and Sgr B2(M) (left three panels). In each panel, the velocity scale is appropriate for the emission in the respective water transition, which was in all cases observed in the upper sideband (USB). The water emission appears at LSR velocities close to the systemic velocities of the sources in question. The dashed lines mark the velocity centroids of the water emission. In addition to the water line, in all spectra emission from other molecular lines is observed. Effective velocity resolutions are 1.52, 1.13, and 1.05 km s-1 for the 325, 439, and 471 H 2O lines. Spectra of the 325, 437, 439, and 471 GHz H2O transitions toward the Mira variable U Her are also shown (right panel). Effective velocity resolutions are 1.52,1.13,1.13, and 1.05 km s-1 for the 325, 437, 439, and 471 GHz H2O lines,,,1.5,,,1,(4.94501217031715 , 0.0218150448536023),G34.2572+0.1532,64.000, 1,G343-02,,283.3283270,1.2499100,34.2580910,0.1527300,,,59,46;68,,~110,1200 (200),MEL93,JCMT,Jy,18 53 18.8,+01 14 59.7,,G34.257+0.153,0,16.000000000,,1992 March 28 - April 1,,6(43)->5(50),0,0,0,,0,,110.000,,34.2580910,0.1527300,283.3283270,1.2499100,,,,,1.1,,,1,(4.94501217031715 , 0.0218150448536023),G34.2572+0.1532,110.000, 1,G343-02,,0.6406910,0.2784090,97.7422010,-60.1810240,,,60,51;65,,36,220 (50),MEL93,JCMT,Jy,00 02 33.8,+00 16 42.3,,G97.742-60.181,0,16.000000000,,1992 March 28 - April 1,,6(42)->5(51),0,0,0,,0,,36.000,,97.7422010,-60.1810240,0.6406910,0.2784090,,,,,1.1,,,1,(0.011182167437895 , 0.00485915371718489),G97.7422-60.1810,36.000, 1,Sgr B2(N),,266.8328720,-28.3723030,0.6768660,-0.0279030,,,~66,50;83,,~300,5000 (200),MEL93,JCMT,Jy,17 47 19.9,-28 22 20.3,,G0.6771-0.0269,1,16.000000000,,1992 March 28 - April 1,,5(15)->4(22),0,0,0,,0,,300.000,,0.6768660,-0.0279030,266.8328720,-28.3723030,,,,,1.5,,,1,(4.65711216895259 , -0.495190103723465),G0.6667-0.0337,300.000, 1,Sgr B2(N),,266.8328720,-28.3723030,0.6768660,-0.0279030,,,~65,50;83,,~380,4300 (730),MEL93,JCMT,Jy,17 47 19.9,-28 22 20.3,,G0.6771-0.0269,1,16.000000000,,1992 March 28 - April 1,,6(43)->5(50),0,0,0,,0,,380.000,,0.6768660,-0.0279030,266.8328720,-28.3723030,,,,,1.1,,,1,(4.65711216895259 , -0.495190103723465),G0.6667-0.0337,380.000, 1,SgrB2(M),,266.8341980,-28.3845190,0.6670210,-0.0352290,,,~60,48;85,,~300,6500 (450),MEL93,JCMT,Jy,17 47 20.2,-28 23 4.3,,G0.6667-0.0344,1,16.000000000,,1992 March 28 - April 1,,5(15)->4(22),0,0,0,,0,,300.000,,0.6670210,-0.0352290,266.8341980,-28.3845190,,Spectra of the 325,439, and 471 GHz H2O transitions (top to bottom) observed toward the star-forming regions G34.3-0.2, W49 N, and Sgr B2(M) (left three panels). In each panel, the velocity scale is appropriate for the emission in the respective water transition, which was in all cases observed in the upper sideband (USB). The water emission appears at LSR velocities close to the systemic velocities of the sources in question. The dashed lines mark the velocity centroids of the water emission. In addition to the water line, in all spectra emission from other molecular lines is observed. Effective velocity resolutions are 1.52, 1.13, and 1.05 km s-1 for the 325, 439, and 471 H 2O lines. Spectra of the 325, 437, 439, and 471 GHz H2O transitions toward the Mira variable U Her are also shown (right panel). Effective velocity resolutions are 1.52,1.13,1.13, and 1.05 km s-1 for the 325, 437, 439, and 471 GHz H2O lines,,,1.5,,,1,(4.65713531201847 , -0.495403313144888),G0.6667-0.0337,300.000, 1,SgrB2(M),,266.8341980,-28.3845190,0.6670210,-0.0352290,,,~60,50;75,,~590,8400 (510),MEL93,JCMT,Jy,17 47 20.2,-28 23 4.3,,G0.6667-0.0344,1,16.000000000,,1992 March 28 - April 1,,6(43)->5(50),0,0,0,,0,,590.000,,0.6670210,-0.0352290,266.8341980,-28.3845190,,,,,1.1,,,1,(4.65713531201847 , -0.495403313144888),G0.6667-0.0337,590.000, 1,SgrB2(M),,0.6406910,0.2784090,97.7422010,-60.1810240,,,~64,48;83,,~220,4100 (180),MEL93,JCMT,Jy,00 02 33.8,+00 16 42.3,,G97.742-60.181,0,16.000000000,,1992 March 28 - April 1,,6(42)->5(51),0,0,0,,0,,220.000,,97.7422010,-60.1810240,0.6406910,0.2784090,,,,,1.1,,,1,(0.011182167437895 , 0.00485915371718489),G97.7422-60.1810,220.000, 1,W49 N,,287.5558560,9.1039860,43.1667780,0.0113790,,,10,-60;70,,1364,33200 (300),MEL93,JCMT,Jy,19 10 13.4,+09 06 14.3,,G43.167+0.011,0,16.000000000,,1992 March 28 - April 1,,5(15)->4(22),0,0,0,,0,,1364.000,,43.1667780,0.0113790,287.5558560,9.1039860,,Spectra of the 325,439, and 471 GHz H2O transitions (top to bottom) observed toward the star-forming regions G34.3-0.2, W49 N, and Sgr B2(M) (left three panels). In each panel, the velocity scale is appropriate for the emission in the respective water transition, which was in all cases observed in the upper sideband (USB). The water emission appears at LSR velocities close to the systemic velocities of the sources in question. The dashed lines mark the velocity centroids of the water emission. In addition to the water line, in all spectra emission from other molecular lines is observed. Effective velocity resolutions are 1.52, 1.13, and 1.05 km s-1 for the 325, 439, and 471 H 2O lines. Spectra of the 325, 437, 439, and 471 GHz H2O transitions toward the Mira variable U Her are also shown (right panel). Effective velocity resolutions are 1.52,1.13,1.13, and 1.05 km s-1 for the 325, 437, 439, and 471 GHz H2O lines,,,1.5,,,1,(5.01879647059069 , 0.158894530755468),G43.1668+0.0106,1364.000, 1,W49 N,,0.6406910,0.2784090,97.7422010,-60.1810240,,,10,-60;70,,191,4170 (230),MEL93,JCMT,Jy,00 02 33.8,+00 16 42.3,,G97.742-60.181,0,16.000000000,,1992 March 28 - April 1,,6(43)->5(50),0,0,0,,0,,191.000,,97.7422010,-60.1810240,0.6406910,0.2784090,,,,,1.1,,,1,(0.011182167437895 , 0.00485915371718489),G97.7422-60.1810,191.000, 1,W49 N,,0.6406910,0.2784090,97.7422010,-60.1810240,,,10,-60;70,,54,1300 (50),MEL93,JCMT,Jy,00 02 33.8,+00 16 42.3,,G97.742-60.181,0,16.000000000,,1992 March 28 - April 1,,6(42)->5(51),0,0,0,,0,,54.000,,97.7422010,-60.1810240,0.6406910,0.2784090,,,,,1.1,,,1,(0.011182167437895 , 0.00485915371718489),G97.7422-60.1810,54.000, 1,W51 Main,,290.9327450,14.5101130,49.4901230,-0.3870570,,,64,50;70,,168,1750 (80),MEL93,JCMT,Jy,19 23 43.9,+14 30 36.4,,G49.488-0.387,0,16.000000000,,1992 March 28 - April 1,,5(15)->4(22),0,0,0,,0,,168.000,,49.4901230,-0.3870570,290.9327450,14.5101130,,,,,1.5,,,1,(5.07773430211507 , 0.253249246686432),G49.4898-0.3876,168.000, 1,W51 Main,,290.9327450,14.5101130,49.4901230,-0.3870570,,,57,50;70,,70,570 (150),MEL93,JCMT,Jy,19 23 43.9,+14 30 36.4,,G49.488-0.387,0,16.000000000,,1992 March 28 - April 1,,6(43)->5(50),0,0,0,,0,,70.000,,49.4901230,-0.3870570,290.9327450,14.5101130,,,,,1.1,,,1,(5.07773430211507 , 0.253249246686432),G49.4898-0.3876,70.000, 1,W51 d,,290.9164450,14.5189280,49.4904310,-0.3689850,,,63,53;70,,188,1170 (120),MEL93,JCMT,Jy,19 23 39.9,+14 31 8.1,,G49.488-0.387,0,16.000000000,,1992 March 28 - April 1,,5(15)->4(22),0,0,0,,0,,188.000,,49.4904310,-0.3689850,290.9164450,14.5189280,,,,,1.5,,,1,(5.077449813447 , 0.253403097459995),G49.4894-0.3690,188.000, 0,Sgr B2(N),,0.6406910,0.2784090,97.7422010,-60.1810240,,,60,,,<180,<1100,MEL93,JCMT,Jy,00 02 33.8,+00 16 42.3,,G97.742-60.181,0,16.000000000,,1992 March 28 - April 1,,6(42)->5(51),0,0,0,,0,,,,97.7422010,-60.1810240,0.6406910,0.2784090,,,,,1.1,,,1,(0.011182167437895 , 0.00485915371718489),G97.7422-60.1810,, 0,W49 N,,287.5558560,9.1039860,43.1667780,0.0113790,,,,-10;40,,,23000 (200),MEL93,JCMT,Jy,19 10 13.4,+09 06 14.3,,G43.167+0.011,0,16.000000000,,1992 March 28 - April 1,,5(15)->4(22),0,0,0,,0,,,,43.1667780,0.0113790,287.5558560,9.1039860,,,,,1.5,,,1,(5.01879647059069 , 0.158894530755468),G43.1668+0.0106,, 0,W49 N,,0.6406910,0.2784090,97.7422010,-60.1810240,,,,-10;40,,,2900 (190),MEL93,JCMT,Jy,00 02 33.8,+00 16 42.3,,G97.742-60.181,0,16.000000000,,1992 March 28 - April 1,,6(43)->5(50),0,0,0,,0,,,,97.7422010,-60.1810240,0.6406910,0.2784090,,,,,1.1,,,1,(0.011182167437895 , 0.00485915371718489),G97.7422-60.1810,, 0,W51 Main,,0.6406910,0.2784090,97.7422010,-60.1810240,,,60,,,<54,<250,MEL93,JCMT,Jy,00 02 33.8,+00 16 42.3,,G97.742-60.181,0,16.000000000,,1992 March 28 - April 1,,6(42)->5(51),0,0,0,,0,,,,97.7422010,-60.1810240,0.6406910,0.2784090,,,,,1.1,,,1,(0.011182167437895 , 0.00485915371718489),G97.7422-60.1810,, 0,W51 d,,290.9164450,14.5189280,49.4904310,-0.3689850,,,60,,,<90,<400,MEL93,JCMT,Jy,19 23 39.9,+14 31 8.1,,G49.488-0.387,0,16.000000000,,1992 March 28 - April 1,,6(43)->5(50),0,0,0,,0,,,,49.4904310,-0.3689850,290.9164450,14.5189280,,,,,1.1,,,1,(5.077449813447 , 0.253403097459995),G49.4894-0.3690,, 0,W51 d,,0.6406910,0.2784090,97.7422010,-60.1810240,,,60,,,<60,<250,MEL93,JCMT,Jy,00 02 33.8,+00 16 42.3,,G97.742-60.181,0,16.000000000,,1992 March 28 - April 1,,6(42)->5(51),0,0,0,,0,,,,97.7422010,-60.1810240,0.6406910,0.2784090,,,,,1.1,,,1,(0.011182167437895 , 0.00485915371718489),G97.7422-60.1810,,

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