engels ohmasersivo://org.gavo.dc/ohmaser/q/scsThe 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/scs/infoIsServedByGAVO Data Center TAP servicehttps://hsweb.hs.uni-hamburg.de/projects/maserdb/http://dc.g-vo.org/ohmaser/q/scs/scs.xml?https://dc.g-vo.org/ohmaser/q/scs/scs.xml?GETapplication/x-votable+xmlRARight Ascension (ICRS decimal)degpos.eq.rarealDECDeclination (ICRS decimal)degpos.eq.decrealSRSearch radiusdegrealfrequencyObserved frequencyMHzem.freqintegerveloc_shellOutflow Velocity of the shell. If vexp is not given in the reference it is calculated.km/sphys.veloc.expansion;pos.bodyrcrealflux_dens_blueFlux Density of the blue-shifted maser peak. For single-peak masers it contains its flux density.Jyphot.flux.density;em.radio.1500-3000MHzrealflux_dens_redFlux Density of the red-shifted maser peak. It contains the flux density for a single peak maser, if it corresponds to the red-shifted peak in other observations.Jyphot.flux.density;em.radio.1500-3000MHzrealresponseformatFile 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.integer180100000true4.19041710.2444450.001http://dc.g-vo.org/ohmaser/q/scs/capabilitieshttps://dc.g-vo.org/ohmaser/q/scs/capabilitieshttp://dc.g-vo.org/ohmaser/q/scs/availabilityhttps://dc.g-vo.org/ohmaser/q/scs/availabilityhttp://dc.g-vo.org/ohmaser/q/scs/tableMetadatahttps://dc.g-vo.org/ohmaser/q/scs/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/scs/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").outputA 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")._rDistance to cone centerdegpos.angDistancedoublenullablemeasure_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.idcharref_keyInternal key for the originating paper, see ohmasers.bibrefs.meta.bibcharnullableraj2000Selected 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.freq16121612.01612.01667.016671.0161216651667intnullableveloc_blueVelocity of the blue-shifted maser peak. For single-peak masers it contains the line velocity.km/sphys.veloc.expansion;pos.bodyrc-374-148.480.3127.645365.20.362944floatnullableveloc_redVelocity of the red-shifted maser peak in km/s. It contains the line velocity for a single peak maser if it corresponds to the red-shifted peak in other observations.km/sphys.veloc.expansion;pos.bodyrc-336.2-123.90822.1151.963319.60.298792floatnullableveloc_centralRadial velocity of the central star. If veloc_central is not given in the reference, it is calculated.km/sphys.veloc.expansion;pos.bodyrc-355.1-1389.4137.508365.20.370926floatnullableveloc_shellOutflow Velocity of the shell. If vexp is not given in the reference it is calculated.km/sphys.veloc.expansion;pos.bodyrc-48.81.413.82487.50.300037floatnullableveloc_errUncertainty of velocity values. Taken from the velocity resolution of the observation. It is actually a lower limit of the uncertainty, because the lines are usually much broader than velocity resolution of the observing equipment.km/sstat.error;phys.veloc.expansion;pos.bodyrc00.10.91.52.270.945441floatnullableflux_dens_flagNULL -- flux density columns contain detections; < -- non-detection at level flux density blue (3 sigma); > -- flux density blue contains a lower limit for the flux; = -- source only gives fluxes; . -- flux density blue contains probable detection; : -- flux density red contains probable detection; & -- both flux densities contain probable detectionsmeta.codecharnullableflux_dens_blueFlux Density of the blue-shifted maser peak. For single-peak masers it contains its flux density.Jyphot.flux.density;em.radio.1500-3000MHz-3.220.020.27.6042419210.977664floatnullableflux_dens_redFlux Density of the red-shifted maser peak. It contains the flux density for a single peak maser, if it corresponds to the red-shifted peak in other observations.Jyphot.flux.density;em.radio.1500-3000MHz-1.330.0380.6927.2852597.280.295643floatnullablemapurlURL to information on an interferometric followup observation for this object.meta.ref.urlcharnullablemonitorurlURL to information on a monitor programme for this object.meta.ref.urlcharnullablera_rawJ2000 RApos.eq.racharnullablede_rawJ2000 Decpos.eq.deccharnullable