engels oh monivo://org.gavo.dc/ohmaser/q/monscsThe GAVO DC teamEngels, D.http://dc.g-vo.org/ohmaser/q/scs/static/uhlogo.pngBunzel, F.2015-09-02T00:00:00Z2015-07-092.4GAVO Data Centre Team

Mönchhofstrasse 12-14, D-69120 Heidelberg

gavo@ari.uni-heidelberg.de+49 6221 54 1837astrophysical-maserssurveysasymptotic-giant-branch-starsA all-sky compilation of galactic stellar sources observed for OH maser emission in the transitions at 1612, 1665, and 1667 MHz. The database contains OH maser observations selected from the literature . These observations belong to more than 6000 different objects. The database consists of three tables: The main table ("masers"), interferometric followup observations ("maps") and monitoring programs ("monitor").2015A&A...582A..68Ehttp://dc.g-vo.org/ohmaser/q/monscs/infoIsServedByGAVO Data Center TAP servicehttp://dc.g-vo.org/ohmaser/q/monscs/scs.xml?https://dc.g-vo.org/ohmaser/q/monscs/scs.xml?GETapplication/x-votable+xmlRARight Ascension (ICRS decimal)degpos.eq.rarealDECDeclination (ICRS decimal)degpos.eq.decrealSRSearch radiusdegrealobs_date_endDate of last observation, Julian yearsyrtime.end;obsrealfrequencyObserved frequencyMHzem.freqintegersource_noUnique, artificial source identifiermeta.codeintegerresponseformatFile format requested for output.meta.code.mimecharmaxrecMaximum number of records returned. Pass 0 to retrieve service parameters.integerverbExhaustiveness of column selection. VERB=1 only returns the most important columns, VERB=2 selects the columns deemed useful to the average user, VERB=3 returns a table with all available columns.integer180100000true75.22000156.1863900.001http://dc.g-vo.org/ohmaser/q/monscs/capabilitieshttps://dc.g-vo.org/ohmaser/q/monscs/capabilitieshttp://dc.g-vo.org/ohmaser/q/monscs/availabilityhttps://dc.g-vo.org/ohmaser/q/monscs/availabilityhttp://dc.g-vo.org/ohmaser/q/monscs/tableMetadatahttps://dc.g-vo.org/ohmaser/q/monscs/tableMetadatahttp://dc.g-vo.org/taphttps://dc.g-vo.org/tap1/0,2,13,21,23,28,30-31,41 2/4,7,12-14,16,18,24-25,33,36-37,43,46,48,50-51,56-57,60-62,67,69,71,73-75,77,79-81,83,89-91,96,99,102,105,108-109,117-119,144-145,147-149,153-156,158-159,161-163,168-169,172-173,178,183,186-188,190 3/20-21,23-25,60,62-63,68-69,71,76-77,80,82-83,85,87-88,93-95,104,106-107,110-111,114,118-119,121-123,125,127-129,131,136,138-139,141-143,152-153,155-158,160-161,163-166,168-169,171,178,180-181,183,189-190,196,198-199,232-233,235-237,239,252-253,255,257,259,262-263,266,273,281-282,288,291,305-307,312,314-315,328-329,331,353-355,388-390,392-394,402-404,406-407,414,416,425,427-429,431,440,442,445,447,464-466,512-514,516-517,520-521,524,526,528,533-536,539-540,543,545-547,553-554,556,558,560,562,564-565,567-568,570,572-574,585-587,600-602,604,606-608,611,628-629,631,641-643,680,682-685,687,696,698-701,703-704,706-707,709-711,716-718,721,723-724,728,730-731,736,738-739,741-743,757-759,764,766-7671.045e-24 1.104e-24http://dc.g-vo.org/ohmaser/q/monscs/coverageRadioohmaserA all-sky compilation of galactic stellar sources observed for OH maser emission in the transitions at 1612, 1665, and 1667 MHz. The database contains OH maser observations selected from the literature . These observations belong to more than 6000 different objects. The database consists of three tables: The main table ("masers"), interferometric followup observations ("maps") and monitoring programs ("monitor").ohmaser.monitorTable of measurements included from monitoring programs.180measure_noUnique measurement identifiermeta.id;meta.main1410.626837.025691.379999999997341791.0intsource_nameName of the observed source. The name given in the reference is usually kept.meta.idcharsource_noUnique, artificial source identifiermeta.code1222.626038.025500.0341741.0intraj2000Selected best RA, J2000degpos.eq.ra;meta.main0.027341739.2583268.065334.999359.7671doublenullabledej2000Selected best Dec, J2000degpos.eq.dec;meta.main-87.3389-62.369-2.5805360.941186.63691doublenullablefrequencyObserved frequencyMHzem.freq16121612.01612.01667.016671.0intnullableref_keyInternal key for the originating paper, see ohmasers.bibrefs.meta.bibcharnullableobs_date_startDate of the first observation, Julian years.yrtime.start;obs1968.781973.261981.162004.082011.650.99631doublenullableobs_date_endDate of last observation, Julian yearsyrtime.end;obs1972.331972.58198820082013.351doublenullablet_resApproximate time resolution of obs_date_*yrtime.resolution0.0050.0050.0050.110.99631floatnullablemax_flux_dens_flag< if max_flux_dens_peak is a 3σ upper limit.meta.codecharnullablemax_flux_dens_peakMaximal flux density observed (or 3σ upper limit)Jyphot.flux.density;em.radio;stat.max0.060.122414.15298.5096070.566667floatnullablemin_flux_dens_flag< if min_flux_dens_peak is a 3σ upper limit.meta.codecharnullablemin_flux_dens_peakMinimal flux density observed (or 3σ upper limit)Jyphot.flux.density;em.radio;stat.min0.30.4047.7212.724425.20.472222floatnullableohmaser.maserssource_nosource_no