ivo://cavity.caha.es/tapCAVITY ProjectCAVITY Project2023-10-10T00:00:00ZCAVITY

UGR, Granada

cavity@ugr.estapThe TAP Service registry for cavity.caha.es.https://cavity.caha.es/tapCataloghttps://cavity.caha.es/tapadql2.0mysql5.7https://cavity.caha.es/tap/asynchttps://cavity.caha.es/tap/synchttps://cavity.caha.es/tap/capabilitieshttps://cavity.caha.es/tap/tableshttps://cavity.caha.es/tap/examplesdr1This page contains CAVITY DR1 data and catalogues for 100 galaxies in 15 voids.dr1.PPAK_cubesFITS files for CAVITY DR1 galaxiesgalaxyCAVITY IDmeta.id;meta.main;intnameCAVITY namemeta.id;chardateObservation datetime.epoch;charversionPipeline versioncharfileFITS file of the galaxymeta.ref;meta.file;meta.fits;chardr1.PPAK_imagesPPAK footprint, Moment 0, and spectra images of the CAVITY DR1 galaxiesgalaxyCAVITY IDmeta.id;meta.main;intimg_footprintPPAK footprint on the SDSS image of the galaxy.meta.ref;meta.image;charimg_momentMoment 0 map (from 450 to 700 nm) of the galaxy. Center of the galaxy is marked with a red circle. Total exposure time of the galaxy is indicated on the upper part of the map.meta.ref;meta.image;charimg_spectrumSpectrum of the center of the galaxy.meta.ref;meta.image;chardr1.MasterMain physical properties of CAVITY galaxiesgalaxyCAVITY ID [7]meta.id;meta.main;intvoidVoid number [7]meta.id;intraRight ascension [1][degree]pos.eq.rafloatdecDeclination [1][degree]pos.eq.decfloatredshiftRedshift [1]src.redshift;floateffr_fracEffective radius fraction [7]phys.size.radius;arith.ratio;floatmorphologyMorphology type [3]src.morph;floatd25Major axis [7][arcsec]phys.angSize.smajAxis;floatinclInclination [7][degree]src.orbital.inclination;floatpaPosition angle [4][degree]pos.posAng;floatrabsmagAbsolute r-band magnitude [1][mag]phot.mag;floatsbSurface brightness [7][mag·arcsec⁻²]phot.mag.sb;floatg_rColor g-r [1][mag]phot.color;em.opt.B;em.opt.R;floatArGalactic Extinction in r-band [7][mag]phys.absorption.gal;floatM_starLog of stellar mass [6][log(M☉)]phys.mass;floatfluxHIHI line flux density [5][Jy·km·s⁻¹]phot.flux.density;em.line.HI;spect.line;floatvmaxgRotational velocity [4][km·s⁻¹]phys.veloc.rotat;floatlogSFRLog of star formation rate [6][log(M☉·yr⁻¹)]phys.SFR;floatSDSS_IDSDSS ID [2]meta.id.cross;floatdr1.VoidsMain physical properties of CAVITY voidsvoidCAVITY Void IDmeta.id;meta.main;intraRight ascension of the center of the maximal sphere [1][degree]pos.eq.ra;floatdecDeclination of the center of the maximal sphere [1][degree]pos.eq.dec;floatxEquatorial x coordinate of the center of the maximal sphere [1][Mpc/h]pos.cartesian.x;floatyEquatorial y coordinate of the center of the maximal sphere [1][Mpc/h]pos.cartesian.y;floatzEquatorial z coordinate of the center of the maximal sphere [1][Mpc/h]pos.cartesian.z;floatrRadius of the maximal sphere [1][Mpc/h]pos.spherical.r;floatvolxEquatorial x coordinate of the center of the void region [1][Mpc/h]pos.cartesian.x;floatvolyEquatorial y coordinate of the center of the void region [1][Mpc/h]pos.cartesian.y;floatvolzEquatorial z coordinate of the center of the void region [1][Mpc/h]pos.cartesian.z;floateffrRadius of the sphere which has the same volume as the void region [1][Mpc/h]pos.spherical.r;floatnumgalsNumber of volume limited galaxies that reside in the entire void region [1]meta.number;intdr1.AGGalactic extinction data for CAVITY galaxiesgalaxyCAVITY IDmeta.id;meta.main;intLEDAGalactic extinction in B-band (ag from Hyperleda catalogue) [3][mag]phys.absorption.gal;em.opt.B;floatSDSS_uGalactic extintion using SDSS U-Band filter [4][mag]phys.absorption.gal;em.opt.U;floatSDSS_gGalactic extintion using SDSS G-Band filter [4][mag]phys.absorption.gal;em.opt.B;floatSDSS_rGalactic extintion using SDSS R-Band filter [4][mag]phys.absorption.gal;em.opt.R;floatSDSS_iGalactic extintion using SDSS I-Band filter [4][mag]phys.absorption.gal;em.opt.I;floatSDSS_zGalactic extintion using SDSS Z-Band filter [4][mag]phys.absorption.gal;em.opt.I;floatdr1.ALFALFA_SDSSALFALFA-SDSS Galaxy Catalogue for CAVITY galaxiesgalaxyCAVITY IDmeta.id;meta.main;intAGCEntry number in the AGC cataloguemeta.id.cross;intVhelioHeliocentric velocity of the HI profile midpoint [1][km·s⁻¹]spect.dopplerVeloc;em.line.HI;intW50Width at 50% level [1][km·s⁻¹]intW20Width at 20% level [1][km·s⁻¹]intHIfluxHI line flux density [1][Jy·km·s⁻¹]phot.flux.density;em.line.HI; spect.line;floatsigfluxUncertainty in HIflux [1][Jy·km·s⁻¹]stat.error;phot.flux.density;floatDistDistance used in MHI, Mstar, SFR [1][Mpc]floatsigDistUncertainty of Dist [1][Mpc]floatlogMHHI mass, where distance is the one adopted in [1][log(M☉)]phys.mass;floatlogMH_errUncertainty in logMH [1]stat.error;phys.mass;floatHicodeHI source code. Good S/N or tentative detection (1 or 2, respectively) [1]intlogMstarTaylorStellar mass from SDSS optical photometry using the Taylor method [2][log(M☉)]phys.mass;floatlogMstarTaylor_errUncertainty in logMstarTaylor [2]stat.error;phys.mass;floatlogMstarMcGaughStellar mass from infrared unWISE photometry using the McGaugh method [2][log(M☉)]phys.mass;floatlogMstarMcGaugh_errUncertainty in logMstarMcGaugh [2]stat.error;phys.mass;floatlogMstarGSWLCStellar mass from GSWLC-2 [2][log(M☉)]phys.mass;floatlogMstarGSWLC_errUncertainty in logMstarGSWLC [2]stat.error;phys.mass;floatlogSFR22Star Formation Rate (SFR) from unWISE infrared photometry using the flux at the frequency of 22 μm [2][log(M☉·yr⁻¹)]phys.SFR;floatlogSFR22_errUncertainty in SFR22 [2]stat.error;phys.SFR;floatlogSFRNUVIRCorrected near-ultraviolet SFR from GALEX NUV photometry SFRNUVcor for galaxies with NUV fluxes available in NASA-Sloan Atlas [2][log(M☉·yr⁻¹)]phys.SFR;floatlogSFRNUVIR_errUncertainty in logSFRNUVIR [2]stat.error;phys.SFR;floatlogSFRGSWLCSFR from GSWLC-2 [2][log(M☉·yr⁻¹)]phys.SFR;floatlogSFRGSWLC_errUncertainty in logSFRGSWLC [2]stat.error;phys.SFR;floatdr1.IFUA catalogue of available IFU data for CAVITY galaxies from other surveysgalaxyCAVITY ID [3]meta.id;meta.main;intCALIFAFlag for CALIFA galaxies in CAVITY [1]meta.code;intMaNGAFlag for MaNGA galaxies in CAVITY [2]meta.code;intdr1.LEDAHyperleda catalogue for CAVITY galaxiesgalaxyCAVITY IDmeta.id;meta.main;intpgcLEDA internal numbermeta.id.cross;intnameLEDA search stringmeta.id;charobjnamePrincipal designationmeta.id;chard25Major axis[arcsec]phys.angSize.smajAxis;floatobjtypeType of object (G=galaxy; S=Star ...)meta.code;charal1950RA 1950 (hours decimal value)pos.eq.ra;floatde1950DEC 1950 (hours decimal value)pos.eq.dec;floatal2000RA 2000 (hours decimal value)pos.eq.ra;floatde2000DEC 2000 (hours decimal value)pos.eq.dec;floatl2Galactic longitude[degree]pos.galactic.lon;floatb2Galactic latitude[degree]pos.galactic.lat;floatsglSupergalactic longitude[degree]pos.supergalactic.lon;floatsgbSupergalactic latitude[degree]pos.supergalactic.lat;floattypeMorphological typemeta.code;src.morph.type;charbarBar (B or blank)meta.code;src.morph.param;charringRing (R or blank)meta.code;src.morph.param;charmultipleMultiple (M or blank)meta.code;src.morph.param;charcompactnessCompactness (C=Compact or D=Diffuse or blank)meta.code;src.morph.param;chartMorphological type codesrc.morph.type;floate_tActual error on tstat.error;src.morph.type;floatlogd25log10 of apparent diameter (d25 in 0.1")[log(arcsec)]phys.size.diameter;floate_logd25Actual error on logd25[log(arcsec)]stat.error;phys.size.diameter;floatlogr25log10 of axis ratio (major axis/minor axis)phys.size.axisRatio;floate_logr25Actual error on logr25stat.error;phys.size.axisRatio;floatpaMajor axis position angle (North Eastwards)[degrees]pos.posAng;floatbriefMean effective surface brightness[mag·arcsec⁻²]phot.mag.sb;stat.mean;floate_briefActual error on brief[mag·arcsec⁻²]stat.error;phot.mag.sb;stat.mean;floatbtTotal B-band magnitude[mag]phot.mag;em.opt.B;floate_btActual error on bt[mag]stat.error;phot.mag;em.opt.B;floatitTotal I-band magnitude[mag]phot.mag;em.opt.I;floate_itActual error on it[mag]stat.error;phot.mag;em.opt.I;floatutTotal U-band magnitude[mag]phot.mag;em.opt.U;floatvmaxgApparent maximum rotation velocity of gas[km·s⁻¹]phys.veloc.rotat;stat.max;floate_vmaxgActual error on vmaxg[km·s⁻¹]stat.error;phys.veloc.rotat;floatm2121-cm line flux in magnitude (see definition in [1])[mag]phys.flux;em.line.HI;floate_m21Actual error on m21[mag]stat.error;phot.flux;em.line.HI;floatmfirFar infrared magnitude (see definition in [1])[mag]phot.mag;floatvradHeliocentric radial velocity from radio measurements[km·s⁻¹]spect.dopplerVeloc.radio;pos.heliocentric;floate_vradActual error on vrad[km·s⁻¹]stat.error;spect.dopplerVeloc.radio;floatvoptHeliocentric radial velocity from optical measurements[km·s⁻¹]spect.dopplerVeloc.opt;pos.heliocentric;floate_voptActual error on vopt[km·s⁻¹]stat.error;spect.dopplerVeloc.opt;floataiInternal extinction in B magnitude (see [1])[mag]phys.absorption;em.opt.B;floatinclInclination[degree]src.orbital.inclination;floata2121-cm self absortion[mag]phys.absorption;em.line.HI;floatlogdclog10 of apparent corrected diameter (dc in 0.1')[log(arcmin)]phys.size.diameter;floatbtcTotal apparent corrected B-magnitude[mag]phot.mag;em.opt.B;floatbri25Mean surface brightness within isophote 25[mag·arcsec⁻²]phot.mag.sb;stat.mean;floatvrotMaximum velocity rotation corrected for inclination[km·s⁻¹]phys.veloc.rotat;stat.max;floate_vrotActual error on vrot[km·s⁻¹]stat.error;phys.veloc.rotat;floatm21cCorrected 21-cm line flux in magnitude (see [1])[mag]phys.flux;phot.mag;em.line.HI;floathic21-cm color index = m21c – btc[mag]phot.color;em.line.HI;em.opt.B;floatvlgRadial velocity (cz) with respect to the Local Group[km·s⁻¹]spect.dopplerVeloc;floatvgsrRadial velocity (cz) with respect to the GSR[km·s⁻¹]spect.dopplerVeloc;floatvvirRadial velocity (cz) corrected for Virgocentric infall[km·s⁻¹]spect.dopplerVeloc;floatv3kRadial velocity (cz) with respect to the CMB radiation[km·s⁻¹]spect.dopplerVeloc;floatmodzRedshift distance modulus[mag]phot.mag.distMod;floatmod0True distance modulus (from parameters)[mag]phot.mag.distMod;floatmabsAbsolute B-magnitude[mag]phys.magAbs;em.opt.B;floatf_astromPrecision flag on celestial positionchare_mod0Actual error on mod0[mag]stat.error;phot.mag.distMod;floate_modzActual error on modz[mag]stat.error;phot.mag.distMod;floate_mabsActual error on mabs[mag]stat.error;phys.magAbs;floatmodbestTrue distance modulus, combining mod0 and modz[mag]phot.mag.distMod;floate_modbestActual error on modbest[mag]stat.error;phot.mag.distMod;floatktTotal K-band magnitude[mag]phot.mag;em.IR.K;floate_ktActual error on kt[mag]stat.error;phot.mag;em.IR.K;floate_utActual error on ut[mag]stat.error;phot.mag;em.opt.U;floathl_names(pgc)List of all namesmeta.id;charcelposb(pgc)B1950 position (character string)pos;charcelposj(pgc)J2000 position (character string)pos;chardr1.MPAMPA-JHU catalogue for CAVITY galaxiesgalaxyCAVITY IDmeta.id;meta.main;intbestObjIDUnique ID in SDSS databasemeta.id;meta.corr;charspecObjIDSpectral ID in SDSS databasemeta.id;meta.corr;charsn_medianMedian S/N per pixel of the whole spectrum [from galSpecInfo]stat.snr;stat.median;floatoii_3726_flux[OII]3726 Flux from Gaussian fit to continuum subtracted data.[10⁻¹⁷·erg·cm⁻²·s⁻¹]phot.flux;floatoii_3726_flux_errUncertainty in oii_3726_flux[10⁻¹⁷·erg·cm⁻²·s⁻¹]stat.error;phot.flux;floatoii_3729_flux[OII]3729 Flux from Gaussian fit to continuum subtracted data.[10⁻¹⁷·erg·cm⁻²·s⁻¹]phot.flux;floatoii_3729_flux_errUncertainty in oii_3729_flux[10⁻¹⁷·erg·cm⁻²·s⁻¹]stat.error;phot.flux;floath_beta_fluxHβ Flux from Gaussian fit to continuum subtracted data.[10⁻¹⁷·erg·cm⁻²·s⁻¹]phot.flux;floath_beta_flux_errUncertainty in the h_beta_flux[10⁻¹⁷·erg·cm⁻²·s⁻¹]stat.error;phot.flux;floatoiii_5007_flux[OIII]5007 Flux from Gaussian fit to continuum subtracted data.[10⁻¹⁷·erg·cm⁻²·s⁻¹]phot.flux;floatoiii_5007_flux_errUncertainty in oiii_5007_flux[10⁻¹⁷·erg·cm⁻²·s⁻¹]stat.error;phot.flux;floath_alpha_contContinuum at line center from 200 pixel median smoothing of the emission-line subtracted continuum[10⁻¹⁷·erg·cm⁻²·s⁻¹·Å⁻¹]phot.flux;spect.continuum;floath_alpha_cont_errUncertainty in h_alpha_cont[10⁻¹⁷·erg·cm⁻²·s⁻¹·Å⁻¹]stat.error;phot.flux;floath_alpha_reqwThe equivalent width of the continuum-subtracted emission line computed from straight integration over the bandpasses listed in [galSpecLine] (emission is negative). In this case the continuum comes from a running 200 pixel median and does not properly account for stellar absorption. In general the EQW measurements provide a better measure of the true equivalent width. The purpose of this measurement is to help characterize the stellar absorption effecting the line. (EW_stellar = REQW – EQW)Åspect.line.eqWidth;spect.continuum;floath_alpha_reqw_errUncertainty in h_alpha_reqwÅstat.error;spect.line.eqWidth;floath_alpha_eqwThe equivalent width of the CB08 continuum-subtracted emission line computed from straight integration over the bandpasses listed in [galSpecLine] (emission is negative). This properly takes into account stellar absorption. Note that it will not be correct in the case of blended lines (i.e., NII & Hα)Åspect.line.eqWidth;spect.continuum;floath_alpha_eqw_errUncertainty in h_alpha_eqwÅstat.error;spect.line.eqWidth;floath_alpha_fluxHα Flux from Gaussian fit to continuum subtracted data.[10⁻¹⁷·erg·cm⁻²·s⁻¹]phot.flux;floath_alpha_flux_errUncertainty in h_alpha_flux[10⁻¹⁷·erg·cm⁻²·s⁻¹]stat.error;phot.flux;floatnii_6584_flux[NII]6584 Flux from Gaussian fit to continuum subtracted data.[10⁻¹⁷·erg·cm⁻²·s⁻¹]phot.flux;floatnii_6584_flux_errUncertainty in nii_6584_flux[10⁻¹⁷·erg·cm⁻²·s⁻¹]stat.error;phot.flux;floatsii_6717_flux[SII]6717 Flux from Gaussian fit to continuum subtracted data.[10⁻¹⁷·erg·cm⁻²·s⁻¹]phot.flux;floatsii_6717_flux_errUncertainty in sii_6717_flux[10⁻¹⁷·erg·cm⁻²·s⁻¹]stat.error;phot.flux;floatsii_6731_flux[SII]6731 Flux from Gaussian fit to continuum subtracted data.[10⁻¹⁷·erg·cm⁻²·s⁻¹]phot.flux;floatsii_6731_flux_errUncertainty in sii_6731_flux[10⁻¹⁷·erg·cm⁻²·s⁻¹]stat.error;phot.flux;floatoh_p16The 16th percentile of the Oxygen abundance derived using Charlot & Longhetti models. The values are reported as 12 + Log O/H. See Tremonti et al (2004) and Brinchmann et al (2004) for details. [from galSpecExtra]phys.abund;stat.median;floatoh_p50The median estimate of the Oxygen abundance derived using Charlot & Longhetti models. The values are reported as 12 + Log O/H. See Tremonti et al (2004) and Brinchmann et al (2004) for details. [from galSpecExtra]phys.abund;stat.median;floatoh_p84The 84th percentile of the Oxygen abundance derived using Charlot & Longhetti models. The values are reported as 12 + Log O/H. See Tremonti et al (2004) and Brinchmann et al (2004) for details. [from galSpecExtra]phys.abund;stat.median;floatlgm_tot_p16The 16th percentile of the Log total stellar mass PDF using model photometry. [from galSpecExtra][log(M☉)]phys.mass;stat.median;floatlgm_tot_p50The median estimate of the Log total stellar mass PDF using model photometry. [from galSpecExtra][log(M☉)]phys.mass;stat.median;floatlgm_tot_p84The 84th percentile of the Log total stellar mass PDF using model photometry. [from galSpecExtra][log(M☉)]phys.mass;stat.median;floatsfr_tot_p16The 16th percentile of the Log total SFR PDF. This is derived by combining emission line measurements from within the fibre where possible and aperture corrections are done by fitting models ala Gallazzi et al (2005), Salim et al (2007) to the photometry outside the fibre. For those objects where the emission lines within the fibre do not provide an estimate of the SFR, model fits were made to the integrated photometry. [from galSpecExtra][log(M☉·yr⁻¹)]phys.SFR;stat.median;floatsfr_tot_p50The median estimate of the Log total SFR PDF. This is derived by combining emission line measurements from within the fibre where possible and aperture corrections are done by fitting models ala Gallazzi et al (2005), Salim et al (2007) to the photometry outside the fibre. For those objects where the emission lines within the fibre do not provide an estimate of the SFR, model fits were made to the integrated photometry. [from galSpecExtra][log(M☉·yr⁻¹)]phys.SFR;stat.median;floatsfr_tot_p84The 84th percentile of the Log total SFR PDF. This is derived by combining emission line measurements from within the fibre where possible and aperture corrections are done by fitting models ala Gallazzi et al (2005), Salim et al (2007) to the photometry outside the fibre. For those objects where the emission lines within the fibre do not provide an estimate of the SFR, model fits were made to the integrated photometry. [from galSpecExtra][log(M☉·yr⁻¹)]phys.SFR;stat.median;floatspecsfr_tot_p16The 16th percentile of the Log total SPECSFR PDF. This is derived by combining emission line measurements from within the fibre where possible and aperture corrections are done by fitting models ala Gallazzi et al (2005), Salim et al (2007) to the photometry outside the fibre. For those objects where the emission lines within the fibre do not provide an estimate of the SFR, model fits were made to the integrated photometry. [from galSpecExtra][log(yr⁻¹)]phys.SFR;stat.median;floatspecsfr_tot_p50The median estimate of the Log total SPECSFR PDF. This is derived by combining emission line measurements from within the fibre where possible and aperture corrections are done by fitting models ala Gallazzi et al (2005), Salim et al (2007) to the photometry outside the fibre. For those objects where the emission lines within the fibre do not provide an estimate of the SFR, model fits were made to the integrated photometry. [from galSpecExtra][log(yr⁻¹)]phys.SFR;stat.median;floatspecsfr_tot_p84The 84th percentile of the Log total SPECSFR PDF. This is derived by combining emission line measurements from within the fibre where possible and aperture corrections are done by fitting models ala Gallazzi et al (2005), Salim et al (2007) to the photometry outside the fibre. For those objects where the emission lines within the fibre do not provide an estimate of the SFR, model fits were made to the integrated photometry. [from galSpecExtra][log(yr⁻¹)]phys.SFR;stat.median;floatd4000_n4000AA break, Balogh et al (1999) definition. [from galSpecIndx]phot.flux.density;arith.ratio;floatd4000_n_errUncertainty in d4000_nstat.error;phot.flux.density;arith.ratio;floatdr1.MorphoThe morphological classification catalogue of CAVITY galaxiesgalaxyCAVITY ID [5]meta.id;meta.main;intGZ1EllGZ1 catalogue of ELLIPTICAL classified galaxy. Ellipticals are marked as 1, else as 0 [1]meta.code;src.morph.type;floatGZ1SGZ1 catalogue of SPIRAL classified galaxy. Spirals are marked as 1, else as 0 [1]meta.code;src.morph.type;floatGZ1UGZ1 catalogue of UNCERTAIN classified galaxy. Galaxies with high uncertainty in classification are marked as 1, else as 0 [1]meta.code;src.morph.type;floatGZ2classThe most common morphology for galaxies among different classifications [2]meta.code.class;src.morph.type;charGZ2formulaGZ2 morphology classification [2]src.morph.type;floatpdominantWeighted fraction of GZ2 votes for “dominant bulge”. Galaxies with dominant bulge have higher values [2]stat.value;floatpnobulgeWeighted fraction of GZ2 votes for “no bulge”. Galaxies with no bulge have higher values [2]stat.value;floatpobviousWeighted fraction of GZ2 votes for “obvious bulge”. Galaxies with obvious bulge have higher values [2]stat.value;floatprobaEarlyProbability of a galaxy being a early-type galaxy (’probaEarly’ = ’probaE’ + ’probaS0’) [3]stat.probability;floatprobaEllProbability of a galaxy being elliptical [3]stat.probability;floatprobaLateProbability of a galaxy being a late-type galaxy (’probaLate’ = ’probaSab’ + ’probaScd’) [3]stat.probability;floatprobaS0Probability of a galaxy being lenticular [3]stat.probability;floatprobaSabProbability of a galaxy being spiral Sa or Sb type [3]stat.probability;floatprobaScdProbability of a galaxy being spiral Sc or Sd type [3]stat.probability;floatTType_DST-type, early–type galaxies are marked with values ≤ 0 and late–type–galaxies with values > 0 [4]meta.code.class;src.morph.type;floatdr1.PAN_MAGLIMThe original Pan catalogue for CAVITY galaxiesgalaxyCAVITY IDmeta.id;meta.main;intraRight Ascension of the galaxy [1][degree]pos.eq.ra;floatdecDeclination of the galaxy [1][degree]pos.eq.dec;floatredshiftRedshift of the void galaxy [1]src.redshift;floatdistComoving distance to the void galaxy [1][Mpc/h]pos.distance;floatrabsmagr-band absolute magnitude of the void galaxy [1][mag]phys.magAbs;em.opt.R;floatg-rg-r band color of the void galaxy [1][mag]phot.color;em.opt.B;em.opt.R;floatxEquatorial x coordinate of the void galaxy [1][Mpc/h]pos.cartesian.x;floatyEquatorial y coordinate of the void galaxy [1][Mpc/h]pos.cartesian.y;floatzEquatorial z coordinate of the void galaxy [1][Mpc/h]pos.cartesian.z;floatplateSDSS plate number [1]meta.number;instr.plate;intfiberSDSS fiber number [1]meta.number;intmjdModified Julian date of the observation [1][day]time.epoch;obs;intdr1.SDSSSDSS photometric catalogue for CAVITY galaxiesgalaxyCAVITY IDmeta.id;meta.main;intobjIDUnique SDSS identifier composed from [skyVersion,rerun,run,camcol,field,obj]meta.id;meta.corr;charpetroR50_rRadius containing 50% of Petrosian flux in the R-band [1][arcsec]phys.size.radius;em.opt.R;floatpetroR50Err_rError in petroR50_r [1][arcsec]stat.error;phys.size.radius;em.opt.R;floatpetroR90_rRadius containing 90% of Petrosian flux in the R-band [1][arcsec]phys.size.radius;em.opt.R;floatpetroR90Err_rError in petroR90_r [1][arcsec]stat.error;phys.size.radius;em.opt.R;floatexpAB_rExponential fit b/a in the R-band [1]phys.size.axisRatio;em.opt.R;floatexpABErr_rError in expAB_r [1]stat.error;phys.size.axisRatio;em.opt.R;floatmodelMag_uModel magnitude in u filter [1][mag]phot.mag;em.opt.U;floatmodelMag_gModel magnitude in g filter [1][mag]phot.mag;em.opt.B;floatmodelMag_rModel magnitude in r filter [1][mag]phot.mag;em.opt.R;floatmodelMag_iModel magnitude in i filter [1][mag]phot.mag;em.opt.I;floatmodelMag_zModel magnitude in z filter [1][mag]phot.mag;em.opt.I;floatmodelMagErr_uError in modelMag_u [1][mag]stat.error;phot.mag;em.opt.U;floatmodelMagErr_gError in modelMag_g [1][mag]stat.error;phot.mag;em.opt.B;floatmodelMagErr_rError in modelMag_r [1][mag]stat.error;phot.mag;em.opt.R;floatmodelMagErr_iError in modelMag_i [1][mag]stat.error;phot.mag;em.opt.I;floatmodelMagErr_zError in modelMag_z [1][mag]stat.error;phot.mag;em.opt.I;float