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VOL06 - Spectral observations of OH and water maser sources at the Crimean Astrophysical Observatory with the RT-22 radio telescope

Short title: Volvach et al. (2006)
Authors: Volvach, L. N.Volvach, A. E.Strepka, I. D.
Journal: Astronomical and Astrophysical Transactions, vol. 25, Issue 5, p.379-384
Bibcode:

Target type: High_mass_SFR

Abstract
Observations of almost all know cosmic masers from decimetre to millimetre wavebands have been performed at the Radio Astronomy Laboratory of the Crimean Astrophysical Observatory with the 22 m radio telescope RT-22. Modernization of existing receivers was performed and also receiving systems were created with maximum possible sensitivities in new frequency ranges that were selected from observations of the least studied maser sources with the 5 GHz room-temperature and cryoelectronic radiometers in the single-antenna mode observations of star-forming regions were conducted using the spectral line of the OH molecule at a frequency of 4765 MHz with a spectral resolution of 0.06 km s-1. The observations of stars of early and late spectral classes were conducted, and spectra were obtained using the spectral lines of water vapour and the OH molecule at frequencies of 1612, 1665, 1667 and 1720 MHz with a spectral resolution of 0.02 km s-1. In addition, utilizing the 22 GHz cryoelectronic receiver in the single-antenna mode, spectral observations of star-forming regions were conducted, and spectra obtained for the spectral line of water vapour.

Abstract

Observations of almost all know cosmic masers from decimetre to millimetre wavebands have been performed at the Radio Astronomy Laboratory of the Crimean Astrophysical Observatory with the 22 m radio telescope RT-22. Modernization of existing receivers was performed and also receiving systems were created with maximum possible sensitivities in new frequency ranges that were selected from observations of the least studied maser sources with the 5 GHz room-temperature and cryoelectronic radiometers in the single-antenna mode observations of star-forming regions were conducted using the spectral line of the OH molecule at a frequency of 4765 MHz with a spectral resolution of 0.06 km s-1. The observations of stars of early and late spectral classes were conducted, and spectra were obtained using the spectral lines of water vapour and the OH molecule at frequencies of 1612, 1665, 1667 and 1720 MHz with a spectral resolution of 0.02 km s-1. In addition, utilizing the 22 GHz cryoelectronic receiver in the single-antenna mode, spectral observations of star-forming regions were conducted, and spectra obtained for the spectral line of water vapour.

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Detection table from Volvach et al. (2006)

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DSS colored	2MASS colored	WISE colored
SDSS color	IRAC color I1,I2,I4	GLIMPSE 360
PACS color (70-160 um)	SPIRE color (250-500 um)	NVSS (1.4GHz)
ATLASGAL 870 um	ATLASGAL 870 um + Planck	Bolocam 1.1 mm
UKIDSS K Download UKIDSS K FITS	2MASS K Download 2MASS K FITS

select MAX(h2o_data_all.ra_hms) as ra_hms,MAX(h2o_data_all.dec_dms) as dec_dms,MAX(h2o_data_all.source_name) as source_name,MAX(h2o_data_all.ra) as ra,MAX(h2o_data_all.dec) as dec,MAX(h2o_data_all.l) as l,MAX(h2o_data_all.b) as b,MAX(h2o_data_all.grp) as grp,MAX(h2o_data_all.other_name) as other_name,MAX(h2o_data_all.other_desc) as other_desc,BOOL_OR(thermal) as thermal,MAX(h2o_data_all.line) as line,MAX(h2o_data_all.vrange) as vrange,MAX(h2o_data_all.vpeak) as vpeak,MAX(h2o_data_all.peak) as peak,MAX(h2o_data_all.fwhm) as fwhm,MAX(h2o_data_all.int) as int,MAX(h2o_data_all.rms) as rms,MAX(h2o_data_all.units) as units,MAX(h2o_data_all.units_rms) as units_rms,MAX(h2o_data_all.date_txt) as date_txt,MAX(h2o_data_all.telescope_ref) as telescope_ref,MAX(h2o_data_all.telescope_conf) as telescope_conf,MAX(h2o_data_all.v_step) as v_step,MAX(h2o_data_all.beam) as beam,MAX(h2o_data_all.beam_maj) as beam_maj,MAX(h2o_data_all.beam_min) as beam_min,MAX(h2o_data_all.beam_pa) as beam_pa,MAX(h2o_data_all.ref) as ref,MAX(h2o_data_all.list_ref) as list_ref,MAX(h2o_data_all.ascii) as ascii,MAX(h2o_data_all.url) as url,MAX(h2o_data_all.image) as image,MAX(h2o_data_all.image2) as image2,MAX(h2o_data_all.image3) as image3,MAX(h2o_data_all.descr) as descr,MAX(h2o_data_all.id) as id,BOOL_OR(mjy_flag) as mjy_flag,BOOL_OR(rms_mjy_flag) as rms_mjy_flag,MAX(h2o_data_all.dist) as dist,1 as dist_parallax,MAX(h2o_data_all.date_txt) as date_txt,MAX(line_det) as line_det,MAX(type) as type,MAX(simbad_types_cat) as simbad_types_cat FROM h2o_data_all  LEFT JOIN all_objects_withmet ON h2o_data_all.grp=all_objects_withmet.group_name LEFT JOIN object_categories ON all_objects_withmet.group_name = object_categories.group_name_cat AND object_categories.tbl_cat = 'all_objects_withmet' LEFT JOIN transitions ON h2o_data_all.line=transitions."Line"  WHERE ref ilike 'VOL06' AND detected=true AND hide=false GROUP BY ref

select h2o_data_all.ra_hms,h2o_data_all.dec_dms,h2o_data_all.source_name,h2o_data_all.ra,h2o_data_all.dec,h2o_data_all.l,h2o_data_all.b,h2o_data_all.grp,h2o_data_all.other_name,h2o_data_all.other_desc,h2o_data_all.thermal,h2o_data_all.line,h2o_data_all.vrange,h2o_data_all.vpeak,h2o_data_all.peak,h2o_data_all.fwhm,h2o_data_all.int,h2o_data_all.rms,h2o_data_all.units,h2o_data_all.units_rms,h2o_data_all.date_txt,h2o_data_all.telescope_ref,h2o_data_all.telescope_conf,h2o_data_all.v_step,h2o_data_all.beam,h2o_data_all.beam_maj,h2o_data_all.beam_min,h2o_data_all.beam_pa,h2o_data_all.ref,h2o_data_all.list_ref,h2o_data_all.ascii,h2o_data_all.url,h2o_data_all.image,h2o_data_all.image2,h2o_data_all.image3,h2o_data_all.descr,h2o_data_all.id,h2o_data_all.mjy_flag,h2o_data_all.rms_mjy_flag,h2o_data_all.dist,h2o_data_all.dist_parallax,h2o_data_all.date_txt,line_det,type,simbad_types_cat FROM h2o_data_all   LEFT JOIN all_objects_withmet ON h2o_data_all.grp=all_objects_withmet.group_name LEFT JOIN object_categories ON all_objects_withmet.group_name = object_categories.group_name_cat AND object_categories.tbl_cat = 'all_objects_withmet' LEFT JOIN transitions ON h2o_data_all.line=transitions."Line"  WHERE ref ilike 'VOL06' AND detected=true AND hide=false ORDER BY detected DESC,id

Display data from paper

VOL06 - Spectral observations of OH and water maser sources at the Crimean Astrophysical Observatory with the RT-22 radio telescope

View as list of objects

Detection table from Volvach et al. (2006)