High-Resolution Very Large Array Imaging of Sloan Digital Sky Survey
Stripe 82 at 1.4 GHzvlastripe82 coneivo://org.gavo.dc/vlastripe82/q/coneThe GAVO DC teamHodge, J. A.Becker, R. H.White, R. L.Richards, G. T.Zeimann, G. R.2014-12-08T00:00:00ZGAVO Data Center TeamMönchhofstrasse 12-14, D-69120 Heidelberggavo@ari.uni-heidelberg.de++49 6221 54 1837surveysradio-continuum-emission
This is a high-resolution radio survey of the Sloan Digital Sky Survey
(SDSS) Southern Equatorial Stripe, a.k.a. Stripe 82. This 1.4 GHz survey
was conducted with the Very Large Array (VLA) primarily in the
A-configuration, with supplemental B-configuration data to increase
sensitivity to extended structure. The survey has an angular resolution
of 1.''8 and achieves a median rms noise of 52 μJy per beam over 92 deg^2.
The catalog contains 17,969 isolated radio components, for an overall
source density of ∼195 sources/deg^2. See also J.A. Hodge et al,
:bibcode:`2011AJ....142....3H` .https://dc.zah.uni-heidelberg.de/vlastripe82/q/cone/infoIsServedByGAVO Data Center TAP servicehttp://dc.zah.uni-heidelberg.de/vlastripe82/q/cone/formhttps://dc.zah.uni-heidelberg.de/vlastripe82/q/cone/formhttp://dc.zah.uni-heidelberg.de/vlastripe82/q/cone/scs.xml?https://dc.zah.uni-heidelberg.de/vlastripe82/q/cone/scs.xml?GETapplication/x-votable+xmlRARight Ascension (ICRS decimal)degpos.eq.rarealDECDeclination (ICRS decimal)degpos.eq.decrealSRSearch radiusdegrealp_sProbability that the source is spurious (e.g., because of a sidelobe of a nearby bright source).stat.likelihood;obsrealf_peakPeak flux density derived by fitting an elliptical Gaussian model to the source. The uncertainty is given in the rms_nose column.mJy/beamphot.flux.density;em.radio.1500-3000MHz;stat.maxrealimagSDSS i-band magnitude of the closest match in SDSS DR6.magphot.mag;em.opt.IrealresponseformatFile 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.integer180100000true331.308-1.0730.01http://dc.zah.uni-heidelberg.de/vlastripe82/q/cone/availabilityhttps://dc.zah.uni-heidelberg.de/vlastripe82/q/cone/availabilityhttp://dc.zah.uni-heidelberg.de/vlastripe82/q/cone/capabilitieshttps://dc.zah.uni-heidelberg.de/vlastripe82/q/cone/capabilitieshttp://dc.zah.uni-heidelberg.de/vlastripe82/q/cone/tableMetadatahttps://dc.zah.uni-heidelberg.de/vlastripe82/q/cone/tableMetadatahttp://dc.zah.uni-heidelberg.de/taphttps://dc.zah.uni-heidelberg.de/tap4/1114,1125-1126,1177
5/4442,4451-4454,4460,4499,4508,4707,4713-4716,4755-4758,4764
6/17661-17663,17719,17723,17725-17727,17762,17774,17799,17803,17820-17822,17844,17848,17856-17858,17860,17975,17981-17983,17991,17995,18036,18040,18068-18069,18071,18112-18114,18116,18176-18178,18180,18184,18679,18683,18685-18687,18743,18747,18749-18751,18792,18794-18795,18823,18827,18849-18851,18868,18872,18880-18882,18884,19015,19036-19038,19045,19060,19200-192028.637e-25 9.932e-25https://dc.zah.uni-heidelberg.de/vlastripe82/q/cone/coverageRadiovlastripe82High-Resolution Very Large Array Imaging of Sloan Digital Sky Survey
Stripe 82 at 1.4 GHz
This is a high-resolution radio survey of the Sloan Digital Sky Survey
(SDSS) Southern Equatorial Stripe, a.k.a. Stripe 82. This 1.4 GHz survey
was conducted with the Very Large Array (VLA) primarily in the
A-configuration, with supplemental B-configuration data to increase
sensitivity to extended structure. The survey has an angular resolution
of 1.''8 and achieves a median rms noise of 52 μJy per beam over 92 deg^2.
The catalog contains 17,969 isolated radio components, for an overall
source density of ∼195 sources/deg^2. See also J.A. Hodge et al,
:bibcode:`2011AJ....142....3H` .
vlastripe82.stripe82
This is a high-resolution radio survey of the Sloan Digital Sky Survey
(SDSS) Southern Equatorial Stripe, a.k.a. Stripe 82. This 1.4 GHz survey
was conducted with the Very Large Array (VLA) primarily in the
A-configuration, with supplemental B-configuration data to increase
sensitivity to extended structure. The survey has an angular resolution
of 1.''8 and achieves a median rms noise of 52 μJy per beam over 92 deg^2.
The catalog contains 17,969 isolated radio components, for an overall
source density of ∼195 sources/deg^2. See also J.A. Hodge et al,
:bibcode:`2011AJ....142....3H` .17969raj2000Right Ascension, J2000degpos.eq.ra;meta.maindoubleindexednullabledej2000Declination, J2000degpos.eq.dec;meta.maindoubleindexednullablep_sProbability that the source is spurious (e.g., because of a sidelobe of a nearby bright source).stat.likelihood;obsfloatnullablef_peakPeak flux density derived by fitting an elliptical Gaussian model to the source. The uncertainty is given in the rms_nose column.mJy/beamphot.flux.density;em.radio.1500-3000MHz;stat.maxfloatindexednullablef_intIntegrated flux density in mJy derived from the elliptical Gaussian model fit.mJyphot.flux.density;em.radio.1500-3000MHzfloatnullablerms_noiseLocal noise estimate at the source position, calculated by combining the measured noise from all grid images contributing to the coadded map at the source position.mJystat.error;phot.flux.densityfloatnullablesmaj_axFWHM semimajor axis of the elliptical Gaussian model for the source after beam deconvolution. This is zero when the fitted value prior to deconvolution to is smaller than the beam (1.8'') due to noise.degphys.angSize.smajAxis;meta.modelledfloatnullablesmin_axFWHM semiminor axis of the elliptical Gaussian model for the source after beam deconvolution. This is zero when the fitted value prior to deconvolution to is smaller than the beam due to noise.degphys.angSize.sminAxis;meta.modelledfloatnullablepaPosition angle of the elliptical Gaussian model for the source after beam deconvolution, east of north.degpos.posAng;meta.modelledfloatnullablesmaj_ax_rawFWHM semimajor axis of the elliptical Gaussian model before beam deconvolution.degphys.angSize.smajAxisfloatnullablesmin_ax_rawFWHM semiminor axis of the elliptical Gaussian model before beam deconvolution.degphys.angSize.sminAxisfloatnullablepa_rawPosition angle of the elliptical Gaussian model for the source before beam deconvolution, east of north.degpos.posAngfloatnullablefieldThe field name is the name of the coadded image containing the source. Note that the field name encodes the center of the field; field hhmmm+ddmmm is centered at RA = hh mm.m, Dec = +dd mm.m. The letter appended to the field name indicates the last catalog release in which the image was modified.meta.id;obs.fieldcharnullablen_sdssNumber of matching SDSS DR6 objects within 8 arcsec.meta.numberintd_sdssSeparation of the closest match in SDSS DR6.degpos.angDistancefloatnullableimagSDSS i-band magnitude of the closest match in SDSS DR6.magphot.mag;em.opt.Ifloatindexednullablec_sdssSDSS morphological class of the closest match in SDSS DR6; s = stellar, g = nonstellar/galaxy.src.morph.typecharnullablectRow count; this is not part of the original table but was added to satisfy SCS requirements.meta.id;meta.mainint