vlastripe82.striivo://org.gavo.dc/vlastripe82/q/stripe82The GAVO DC teamHodge, J. A.Becker, R. H.White, R. L.Richards, G. T.Zeimann, G. R.2014-12-08T00:00:00ZGAVO Data Centre Team

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gavo@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` .2011AJ....142....3Hhttp://dc.g-vo.org/tableinfo/vlastripe82.stripe824/1114,1125-1126,1177 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-25Radiovlastripe82 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.main9.8081711.06232.6184348.932350.1821doubleindexednullabledej2000Declination, J2000degpos.eq.dec;meta.main-1.39151-1.212730.0009555561.218081.4011doubleindexednullablep_sProbability that the source is spurious (e.g., because of a sidelobe of a nearby bright source).stat.likelihood;obs0.0140.0140.1620.70.8771floatnullablef_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.max0.30.320.7417.0181838.761floatindexednullablef_intIntegrated flux density in mJy derived from the elliptical Gaussian model fit.mJyphot.flux.density;em.radio.1500-3000MHz0.120.341.6934.9762348.241floatnullablerms_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.density0.0360.0520.0640.37515.0581floatnullablesmaj_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.modelled000.0002444440.001083330.00828751floatnullablesmin_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.modelled000.0001486110.0006693890.002931941floatnullablepaPosition angle of the elliptical Gaussian model for the source after beam deconvolution, east of north.degpos.posAng;meta.modelled00901801801floatnullablesmaj_ax_rawFWHM semimajor axis of the elliptical Gaussian model before beam deconvolution.degphys.angSize.smajAxis0.000150.0002472220.000350.001112440.008291671floatnullablesmin_ax_rawFWHM semiminor axis of the elliptical Gaussian model before beam deconvolution.degphys.angSize.sminAxis0.0001472220.0001902780.0002902780.0007152220.002943061floatnullablepa_rawPosition angle of the elliptical Gaussian model for the source before beam deconvolution, east of north.degpos.posAng00901801801floatnullablefieldThe 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.number00.01.04.0251.0intd_sdssSeparation of the closest match in SDSS DR6.degpos.angDistance00.050.557.5180.554566floatnullableimagSDSS i-band magnitude of the closest match in SDSS DR6.magphot.mag;em.opt.I-114.339220.3323.3928.10.554566floatindexednullablec_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.main0539.048984.017428.96179681.0int