pcc coneivo://org.gavo.dc/pcc/q/coneThe GAVO DC teamWittmann, C.Kotulla, R.Lisker, T.Grebel, E.K.Conselice, C.J.Janz, J.Penny, S.J.2019-08-30T00:00:00ZGAVO Data Centre Team

Mönchhofstrasse 12-14, D-69120 Heidelberg

gavo@ari.uni-heidelberg.de+49 6221 54 1837perseus-clustergalaxy-colorsearly-type-galaxiesdwarf-elliptical-galaxies This is a catalog of 5437 morphologically classified sources in the direction of the Perseus galaxy cluster core, among them 496 early-type low-mass galaxy candidates. The catalog is primarily based on V-band imaging data acquired with the William Herschel Telescope. Additionally, we used archival Subaru multiband imaging data in order to measure aperture colors and to perform a morphological classification. The catalog reaches its 50 per cent completeness limit at an absolute V-band luminosity of -12 mag and a V-band surface brightness of 26 mag arcsec^-2 . In addition to the published table, this service also contains cutout images of the objects investigated.2019ApJS..245...10Whttps://dc.g-vo.org/pcc/q/cone/infoCatalogResearchIsServedByGAVO Data Center TAP servicehttp://dc.g-vo.org/pcc/q/cone/scs.xml?https://dc.g-vo.org/pcc/q/cone/scs.xml?GETapplication/x-votable+xmlRARight Ascension (ICRS decimal)degpos.eq.rarealDECDeclination (ICRS decimal)degpos.eq.decrealSRSearch radiusdegrealmagIntegrated V-band apparent magnitude corrected for extinction.magphot.mag;em.opt.Vrealr_50Half-light radius in the V band..arcsecphys.angsizerealmu50Effective V band surface brightness within R_50 corrected for extinctionmag.arcsec**-2phot.mag.sbrealsersic_indexSérsic index, upper limit constrained to 4 (cf. paper, sect. 4.3)stat.fit.paramrealresponseformatFile 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.integer180100000true49.595841.26890.001http://dc.g-vo.org/pcc/q/cone/formhttps://dc.g-vo.org/pcc/q/cone/formhttp://dc.g-vo.org/pcc/q/cone/capabilitieshttps://dc.g-vo.org/pcc/q/cone/capabilitieshttp://dc.g-vo.org/pcc/q/cone/availabilityhttps://dc.g-vo.org/pcc/q/cone/availabilityhttp://dc.g-vo.org/pcc/q/cone/tableMetadatahttps://dc.g-vo.org/pcc/q/cone/tableMetadatahttp://dc.g-vo.org/taphttps://dc.g-vo.org/taphttp://dc.g-vo.org/pcc/q/stamp/dlgethttps://dc.g-vo.org/pcc/q/stamp/dlgethttp://dc.g-vo.org/pcc/q/stamp/dlmetahttps://dc.g-vo.org/pcc/q/stamp/dlmetaGETapplication/x-votable+xml;content=datalinkIDThe publisher DID of the dataset of interestmeta.id;meta.maincharresponseformatFile 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.integerObservatorio del Roque de los MuchachosSubaru telescopeWilliam Herschel TelescopeSubaru Hyper Suprimecam6/1700-1701https://dc.g-vo.org/pcc/q/cone/coverageOpticalpcc This is a catalog of 5437 morphologically classified sources in the direction of the Perseus galaxy cluster core, among them 496 early-type low-mass galaxy candidates. The catalog is primarily based on V-band imaging data acquired with the William Herschel Telescope. Additionally, we used archival Subaru multiband imaging data in order to measure aperture colors and to perform a morphological classification. The catalog reaches its 50 per cent completeness limit at an absolute V-band luminosity of -12 mag and a V-band surface brightness of 26 mag arcsec^-2 . In addition to the published table, this service also contains cutout images of the objects investigated.pcc.main This is a catalog of 5437 morphologically classified sources in the direction of the Perseus galaxy cluster core, among them 496 early-type low-mass galaxy candidates. The catalog is primarily based on V-band imaging data acquired with the William Herschel Telescope. Additionally, we used archival Subaru multiband imaging data in order to measure aperture colors and to perform a morphological classification. The catalog reaches its 50 per cent completeness limit at an absolute V-band luminosity of -12 mag and a V-band surface brightness of 26 mag arcsec^-2 . In addition to the published table, this service also contains cutout images of the objects investigated.object_nameIdentifier from Wittman et al (2019).meta.id;meta.maincharindexedprimaryraICRS Right Ascension from WHT imagedegpos.eq.ra;meta.main49.235549.275249.662249.985150.00891doubleindexednullabledecICRS Declination from WHT imagedegpos.eq.dec;meta.main41.195741.245141.491641.741341.76931doubleindexednullablemagIntegrated V-band apparent magnitude corrected for extinction.magphot.mag;em.opt.V14.0818.711622.5424.0124.31doublenullableerr_magError in integrated apparent magnitude for sources fitted with GALFIT (i.e., pflag = 1 .. 8; NULL otherwise)magstat.error;phot.mag;em.opt.V000.030.130.630.909509floatnullabler_50Half-light radius in the V band..arcsecphys.angsize0.120.120.713.329215.231floatnullableerr_r_50Error in half-light radius in the V band.arcsecstat.error;phys.angsize00.010.040.251.150.845319floatnullablemu50Effective V band surface brightness within R_50 corrected for extinctionmag.arcsec**-2phot.mag.sb15.8520.1522.9625.3926.751floatnullableerr_mu50Error in the effective surface brightness propagated from err_mag and err_r_50mag.arcsec**-2stat.error;phot.mag.sb00.010.130.6710.845319floatnullablesersic_indexSérsic index, upper limit constrained to 4 (cf. paper, sect. 4.3)stat.fit.param0.050.090.823.508441floatnullableerr_sersic_indexError in Sérsic index for sources fitted with GALFIT with free N parameter (pflag = 1)stat.error;stat.fit.param00.010.191.6823.710.581387floatnullableb_aAxis ratio in the V band for sources fitted with GALFIT (pflag = 1 .. 8)phys.angsize;arith.ratio0.10.140.66110.909509floatnullableerr_b_aError in axis ratio for sources fitted with GALFIT with free B/A parameter (pflag = 1 - 4)stat.error;phys.angsize;arith.ratio000.050.280.930.827294floatnullablepaPosition Angle for sources fitted with GALFIT and b_a < 0.9 [North/Up=0, East/Left=90]; from V band.degpos.posang-89.9-82.9-0.983.928900.740298floatnullableerr_paError in position angle.degstat.error;pos.posang00.25.132.92889.30.740298floatnullablea_vV-band galactic foreground extinction.magphys.absorption;em.opt.V0.390.410.450.490.561floatnullablepflagPhotometry processing flag (see note).meta.code11.01.09.091.0shortresflag1 if there were significant residuals after substracting GALFIT model, 0 otherwise. This is only given for sources fitted with GALFIT (i.e., pflag = 1 .. 8)meta.code.qual00.00.01.010.90950894shortnullablebgflagBackground fitted with: ...0: Galfit; ...1: SExtractor with BACK_SIZE = 256 pixel background map, ...2: like 1, but BACK_SIZE = 32 pixelmeta.code00.00.02.021.0shortg_r_1Subaru g-r for aperture 1, color corrected for extinction. (r_aper1 = 1 R50 for sources with R50 > 4 pixels, r_aper1 = 4 pixels for sources with R50 <= 4 pixels)magphot.color;em.opt.V;em.opt.R-0.610.10.781.672.260.992091floatnullableerr_g_r_1Error in g-r for aperture 1magphot.color;em.opt.V;em.opt.R00.010.080.3410.992091floatnullabler_z_1Subaru r-z for aperture 1, color corrected for extinction. (r_aper1 = 1 R50 for sources with R50 > 4 pixels, r_aper1 = 4 pixels for sources with R50 <= 4 pixels)magphot.color;em.opt.R;em.opt.I-0.620.220.71.833.390.988413floatnullableerr_r_z_1Error in r-z for aperture 1magphot.color;em.opt.R;em.opt.I00.010.090.50.990.988413floatnullableg_r_2Subaru g-r for aperture 2, color corrected for extinction. (only for sources with R50 > 4 pixels, where r_aper2 = 2 R50)magphot.color;em.opt.V;em.opt.R-0.730.230.661.49411.940.304212floatnullableerr_g_r_2Error in g-r for aperture 2magphot.color;em.opt.V;em.opt.R00.020.120.730.980.304212floatnullabler_z_2Subaru r-z for aperture 2, color corrected for extinction. (only for sources with R50 > 4 pixels, where r_aper2 = 2 R50)magphot.color;em.opt.R;em.opt.I-0.20.240.541.311.860.290418floatnullableerr_r_z_2Error in r-z for aperture 2magphot.color;em.opt.R;em.opt.I0.010.020.150.8510.290418floatnullableg_r_flag1 if g-r photometry possibly comtaminated through bleeding trails of bright stars within 3 arcsec, 0 otherwisemeta.code.qual00.00.01.010.99209124shortnullabler_z_flag1 if r-z photometry possibly comtaminated through bleeding trails of bright stars within 3 arcsec, 0 otherwisemeta.code.qual00.00.01.010.98841274shortnullablea_gg-band galactic foreground extinction.magphys.absorption;em.opt.V0.480.510.550.60.690.992091floatnullablea_rr-band galactic foreground extinction.magphys.absorption;em.opt.R0.330.350.380.420.480.992459floatnullablea_zz-band galactic foreground extinction.magphys.absorption;em.opt.I0.180.20.210.230.260.988413floatnullablemorphologyMorphological classificationsrc.classcharnullablenucleationRemark on nucleationsrc.classcharnullablecutout_linkLink to a FITS cutout for this source from an r-band mosaic. See datalink for additional retrieval options.meta.ref.urlcharnullable