J/A+A/699/A366ivo://CDS.VizieR/J/A+A/699/A366doi:10.26093/cds/vizier/bc-nv/ldggCDSColombo D.Kalinova V.Bazzi Z.Sanchez S.F.Bolatto A.D.Wong T.,Villanueva V.Mudivarthi N.Rosolowsky E.Weiss A.French K.D.,Leroy A.Barrera-Ballesteros J.Garay-Solis Y.Bigiel F.Tripathi A.,Rodriguez B.2026-08-28T12:49:16Z2025-07-22T10:07:36ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frgalaxiescatalogsmolecular-physicsline-intensitieschemical-abundancesco-line-emissionStudying galaxy evolution requires knowledge not only of the stellar properties, but also of the interstellar medium (in particular the molecular phase) out of which stars form, using a statistically significant and unbiased sample of galaxies. To this end, we introduce here the integrated Extragalactic Database for Galaxy Evolution (iEDGE), a collection of integrated stellar and nebular emission lines, and molecular gas properties from 643 galaxies in the local Universe. These galaxies are drawn from the CALIFA datasets, and are followed up in CO lines by the APEX, CARMA, and ACA telescopes. As this database is assembled from data coming from a heterogeneous set of telescopes (including IFU optical data and single-dish and interferometric CO data), we adopted a series of techniques (tapering, spatial and spectral smoothing, and aperture correction) to homogenise the data. Due to the application of these techniques, the database contains measurements from the inner regions of the galaxies and for the full galaxy extent. We used the database to study the fundamental star formation relationships between star formation rate (SFR), stellar mass (M*), and molecular gas mass (Mmol) across galaxies with different morphologies. We observed that the diagrams defined by these quantities are bi-modal, with early-type passive objects well separated from spiral star-forming galaxies. Additionally, while the molecular gas fraction (fmol=Mmol/M*) decreases homogeneously across these two types of galaxies, the star formation efficiency (SFE=SFR/Mmol) in the inner regions of passive galaxies is almost two orders of magnitude lower compared to the global values. This indicates that inside-out quenching requires not only low fmol, but also strongly reduced SFE in the galactic centres.2025A&A...699A.366Chttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/699/A366CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/648/A64 : Star formation quenching stages of galaxies (Kalinova+ 2021)J/ApJ/846/159 : Interferometric CO obs. of 126 CALIFA galaxiesJ/MNRAS/484/5192 : Molecular gas distribution and star formation (Chown+, 2019)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/699/A366https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/699/A366http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/699/A366https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/699/A366https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/699/A366http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/699/A366GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/699/A366/tablec1 (Integrated CO and optical measurements for 643 local galaxies)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/699/A366/tablec1?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/699/A366/tablec1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/699/A366/tablec1?GETtext/xml+votable180.050000true343.35291674.79950.0055555555555555565/4415 6/0 43 50 56 131 224 425 471 545 552 554 558 568 573 589 620-621 626-627 635 675 721 733 738 907-909 975 995 2130 2206 2229 2248 2251 2254 2272-2274 2290 2641 4053 4114 4167 4178 4279 4342 4416 4445 4454 4472 4477 4507 4511 4526 4647 4654-4655 4667 4688 4696 4704 4712 4716 4719 4753-4754 4772 4799 4801 4806-4807 4813 4829 4840 4843-4844 4850 4912 4950 4957 4993 5024 5028 5148 5190 5247 5298 5332 5579 5593 5701 5889 6162 6212 6214 6216 6240-6241 6261 6270 6342 6362 6366 6977 7214 7309 7340 7559-7560 7584 7591 7822 7824 7834 8045 8195-8196 8297 8323 8327 8331 8341 8366 8376 8391 8458 8477 8479-8480 8492 8498 8509 8511 8522 8536-8537 8552 8557 8562-8563 8570 8589 8605 8621 8626 8646 8656 8667 8673 8700 8705 8719 8723 8728 8743 8752 8754 8825 8883 8898 8900 8919 8921-8922 8973 8984 8992 9098 9101 9124 9187 9216 9220 9287 9368 9381 9622 9628 9718 9798 9812 9875 9882-9883 9885 9891 9946 9974 10025 10111 10113 10200 10213 10220-10221 10240 10280 10286 10379-10381 10398 10400-10401 10414 10422 10515 10566 10583 10588 10595 10612 10627-10629 10705 10739-10740 10752 10773 10778 10846 10987 11044 11070 11112 11164 11196 11272 11290 11326 11369 11372 11374 11377 11383 11392 11435 11443 11525 11544 11832 11905 11944 12306 12378 12455 12497 12508 12532 12566 12585 12709 12794 13128 13316 13350 13380-13381 13459 16007 16696 16702 16787-16788 16793 17233-17234 17237-17238 17350 17392 17398 17486 17492 17499 17502 17509 17511 17516 17520 17571 17578 17667 17672 17736 17745 17747-17748 17751 17758 17761 17767 17773 17817 17819 17912 17998 18008-18009 18049 18069 18071 18081 18173 18209 18214 18226 18241-18242 18252 18295 18300-18302 18381 18383 18523 18653 18775 18779 18781 18790 18800 18838 18854 18922 18929 18931-18932 18934-18935 18939 18941 19027 19062 19073 19084 19108 19186 19227 19260 19267 19283 19303 19325 19387 19417 19432 19458 19487 19489-19490 19508 19515 19536-19538 19589 19593 19618 19633 19642 19661 19671 19678 19696 19749 19751 19848 19897 19928 19939-19940 19954 19981 19983-19984 19991 19993 19996-19997 20009 20014 20020 20023 20031-20033 20040 20140 20193 20254 20279 20282 20303 20356 20372 20417-20418 20429 21857 21862 21872 21953 22353 22356 22361 22364 22651-22652 22654-22655 22737 22740-22742 22826 23023 23051 23072 23076 23182 23204 23206 23208 23273 23294 23337 23353 23356 23401 23405 23895 23916 24055 24227 25520 25715 25770 25888-25890 26055 26102 26108 26125 26318 26340 26432 26451 26495 26548 26551 26563 26932 27133 27259 27368 27559 27567 27596 27608 27719 27725 27729 27738 27748 27761 27767 27830 27849 27853 27861-27862 27910 27912 27914-27915 27926 27938 28019 28067 28075-28076 28112 28149 28169 28221 28230 28249-28251 28263-28264 28272-28273 28294 28310 28322 28365 28430 28458 28491 28497 28513 28522 28579 28617 28639 29973 30044 31218 31348 31356 31478 31537 31546 31551 31628 31642-31643 31688-31689 31736-31737 32400 32462 32471 32478 32482 32555 32559 32561 32572 32602 32614 32682 36604 36733 36765 36793 36797 36805 36857 48880 49084 49121 49130 49150https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/699/A366?format=asciiRadiodefaultJ/A+A/699/A366/tablec1Integrated CO and optical measurements for 643 local galaxiesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintONameAlternative name of the galaxy (Alias)meta.idcharCARMAGlobetamb[-999] CARMA Global main beam efficiency (CARMA_Glob_eta_mb)stat.paramfloatBeammedEWHaBeam median Halpha equivalent width (Beam_med_EWHa)0.1nmpos.angDistance;stat.mediandoubleAPEXBeamRMS? APEX Beam CO noise level (standard deviation of CO spectrum, sigmaRMS) (APEX_Beam_RMS)Kinstr.det.noise;instr.beamdoublenullableACABeamW50m2? ACA Beam full- width half maximum of the CO spectrum calculated via moment 2nd (ACA_Beam_W50_mom2)km/sspect.line.widthdoublenullableACABeamepsobs? ACA Beam statistical error for the CO flux (ACA_Beam_eps_obs)K.km/sstat.error;phot.flux;instr.beamdoublenullableBeamL12W3-7.5? Beam 12um luminosity from WISE W3 at 7.5 arcsec resolution (Beam_L12um_w3_7p5)solLumphys.luminositydoublenullableFinalQSQuenching stage classification (Final_QS) (2)src.classcharFinalNANuclear activity classification (Final_NA) (3)src.classcharSimbadNameSimbad column added by the CDSmeta.idcharnullableRAJ2000Right ascension of the galaxy centre (J2000) (RA)degpos.eq.ra;meta.mainDEJ2000Declination of the galaxy centre (J2000) (DEC)degpos.eq.dec;meta.mainVlsrLSR velocity of the galaxy, derived from the stellar redshift (Vlsr)km/sphys.veloc;src.class.starGalaxy;pos.lsrdoublezstarStellar redshift of the galaxy (zstar)src.redshift;pos.heliocentricdoubleDistanceDistance to the galaxy (Distance)Mpcpos.distancedoubleInclGalaxy inclination (Incl)degsrcdoublePAGalaxy position angle (PA)degpos.posAngdoubleReGalaxy effective radius (Re_as)arcsecphys.angSizedoubleGlobmedEWHaGlobal median Halpha equivalent width (Glob_med_EWHa)0.1nmspect.line.eqWidth;stat.mediandoubleGlobMstarGlobal stellar mass (Glob_Mstar)solMassphys.massdoubleGlobSFRGlobal star formation rate derived using Balmer decrement (Glob_SFR)solMass/yrmeta.iddoubleGlobsSFR? Global specific star formation rate (Glob_sSFR)yr**-1phys.SFRdoublenullablee_GlobMstarGlobal uncertainty on the stellar mass (Err_Glob_Mstar)solMassphys.massdoublee_GlobSFRGlobal uncertainty on the star formation rate derived using Balmer decrement (Err_Glob_SFR)solMass/yrstat.errordoublee_GlobsSFR? Global uncertainty on the specific star formation rate (Err_Glob_sSFR)yr**-1stat.errordoublenullableGlobGasMetGlobal gas-phase metallicity derived via the O3N2 method (Glob_Gas_Met)phys.abund.ZdoubleGlobaco10b13Global CO(1-0)-to-H2 conversion factor (Glob_alpha_co10_b13) (1)solMass.K**-1.km**-1.s.pc**-2arith.factordoubleGlobR21Global CO(2-1)/CO(1-0) flux ratio derived from the star formation rate surface density (Glob_R21)phot.flux;arith.ratiodoubleAPEXGlobk2jyb[-999] APEX Global Jy/beam per Kelvin (APEX_Glob_k2jypb)Jy.K**-1.beam**-1arith.factorfloatAPEXGlobetamb? APEX Global main beam efficiency (APEX_Glob_eta_mb)stat.paramdoublenullableAPEXGlobRMS? APEX Global CO noise level (standard deviation of CO spectrum, sigmaRMS) (APEX_Glob_RMS)Kinstr.det.noisedoublenullableAPEXGlobTpeak? APEX Global peak Tmb across the CO spectrum (APEX_Glob_Tpeak)Kphys.temperaturedoublenullableAPEXGlobSNR? APEX Global signal-to-noise ratio of the CO observation (APEX_Glob_SNR)obs.param;obsdoublenullableAPEXGlobW50m2? APEX Global full-width half maximum of the CO spectrum calculated via moment 2nd (APEX_Glob_W50_mom2)km/sspect.line.widthdoublenullableAPEXGlobepsobs? APEX Global statistical error for the CO flux (APEX_Glob_eps_obs)K.km/sstat.error;phot.flux;spect.linedoublenullableAPEXGlobFco? APEX Global CO flux (APEX_Glob_Fco)Jy.km.s**-1.beam**-1phot.fluxdoublenullableAPEXGlobLco? APEX Global CO luminosity (APEX_Glob_Lco)pc**2.K.km.s**-1phys.luminositydoublenullableAPEXGlobMmol? APEX Global molecular gas mass (APEX_Glob_Mmol)solMassphys.massdoublenullableAPEXGlobfmol? APEX Global molecular gas mass to stellar mass ratio (APEX_Glob_fmol)phys.mass;arith.ratiodoublenullableAPEXGlobSFE? APEX Global star formation efficiency (APEX_Glob_SFE)yr**-1stat.paramdoublenullableCARMAGlobk2jyb? CARMA Global Jy/beam per Kelvin (CARMA_Glob_k2jypb)Jy.K**-1.beam**-1arith.factordoublenullableCARMAGlobRMS? CARMA Global CO noise level (standard deviation of CO spectrum, sigmaRMS) (CARMA_Glob_RMS)Kinstr.det.noisedoublenullableCARMAGlobTpeak? CARMA Global peak Tmb across the CO spectrum (CARMA_Glob_Tpeak)Kphys.temperaturedoublenullableCARMAGlobSNR? CARMA Global signal-to-noise ratio of the CO observation (CARMA_Glob_SNR)obs.param;obsfloatnullableCARMAGlobW50m2? CARMA Global full-width half maximum of the CO spectrum calculated via moment 2nd (CARMA_Glob_W50_mom2)km/sspect.line.widthdoublenullableCARMAGlobepsob? CARMA Global statistical error for the CO flux (CARMA_Glob_eps_obs)K.km/sstat.error;phot.flux;spect.linedoublenullableCARMAGlobFco? CARMA Global CO flux (CARMA_Glob_Fco)Jy.km.s**-1.beam**-1phot.fluxfloatnullableCARMAGlobLco? CARMA Global CO luminosity (CARMA_Glob_Lco)pc**2.K.km.s**-1phys.luminositydoublenullableCARMAGlobMmol? CARMA Global molecular gas mass (CARMA_Glob_Mmol)solMassphys.massdoublenullableCARMAGlobfmol? CARMA Global molecular gas mass to stellar mass ratio (CARMA_Glob_fmol)phys.mass;arith.ratiodoublenullableCARMAGlobSFE? CARMA Global star formation efficiency (CARMA_Glob_SFE)yr**-1stat.paramdoublenullableACAGlobk2jyb? ACA Global Jy/beam per Kelvin (ACA_Glob_k2jypb)Jy.K**-1.beam**-1arith.factordoublenullableACAGlobetamb[-999] ACA Global main beam efficiency (ACA_Glob_eta_mb)stat.paramfloatACAGlobRMS? ACA Global CO noise level (standard deviation of CO spectrum, sigmaRMS) (ACA_Glob_RMS)Kinstr.det.noisedoublenullableACAGlobTpeak? ACA Global peak Tmb across the CO spectrum (ACA_Glob_Tpeak)Kphys.temperaturedoublenullableACAGlobSNR? ACA Global signal-to-noise ratio of the CO observation (ACA_Glob_SNR)obs.param;obsdoublenullableACAGlobW50m2? ACA Global full-width half maximum of the CO spectrum calculated via moment 2nd (ACA_Glob_W50_mom2)km/sspect.line.widthdoublenullableACAGlobepsob? ACA Global statistical error for the CO flux (ACA_Glob_eps_obs)K.km/sstat.error;phot.flux;spect.linedoublenullableACAGlobFco? ACA Global CO flux (ACA_Glob_Fco)Jy.km.s**-1.beam**-1phot.fluxdoublenullableACAGlobLco? ACA Global CO luminosity (ACA_Glob_Lco)pc**2.K.km.s**-1phys.luminositydoublenullableACAGlobMmol? ACA Global molecular gas mass (ACA_Glob_Mmol)solMassphys.massdoublenullableACAGlobfmol? ACA Global molecular gas mass to stellar mass ratio (ACA_Glob_fmol)phys.mass;arith.ratiodoublenullableACAGlobSFE? ACA Global star formation efficiency (ACA_Glob_SFE)yr**-1stat.paramdoublenullableFinalGlobSNRGlobal signal-to-noise ratio of the CO observation from the consolidated sample (Final_Glob_SNR)stat.snrdoubleFinalGlobMmolGlobal molecular gas mass from the consolidated sample (Final_Glob_Mmol)solMassphys.massdoubleFinalGlobfmol? Global molecular gas mass fraction from the consolidated sample (Final_Glob_fmol)phys.mass;arith.ratiodoublenullableFinalGlobSFEGlobal star formation efficiency from the consolidated sample (Final_Glob_SFE)yr**-1stat.paramdoublee_APEXGlobFco? APEX Global uncertainty on the CO flux (APEX_Err_Glob_Fco)Jy.km.s**-1.beam**-1phot.fluxdoublenullablee_APEXGlobLco? APEX Global uncertainty on the CO luminosity (APEX_Err_Glob_Lco)pc**2.K.km.s**-1phys.luminositydoublenullablee_APEXGlobMmol? APEX Global uncertainty on the molecular gas mass (APEX_Err_Glob_Mmol)solMassphys.massdoublenullablee_APEXGlobfmol? APEX Global uncertainty on the molecular gas mass to stellar mass ratio (APEX_Err_Glob_fmol)phys.mass;arith.ratiodoublenullablee_APEXGlobSFE? APEX Global uncertainty on the star formation efficiency (APEX_Err_Glob_SFE)yr**-1stat.paramdoublenullablee_CARMAGlobFco? CARMA Global uncertainty on the CO flux (CARMA_Err_Glob_Fco)Jy.km.s**-1.beam**-1phot.fluxdoublenullablee_CARMAGlobLco? CARMA Global uncertainty on the CO luminosity (CARMA_Err_Glob_Lco)pc**2.K.km.s**-1phys.luminositydoublenullablee_CARMAGlobMmol? CARMA Global uncertainty on the molecular gas mass (CARMA_Err_Glob_Mmol)solMassphys.massdoublenullablee_CARMAGlobfmol? CARMA Global uncertainty on the molecular gas mass to stellar mass ratio (CARMA_Err_Glob_fmol)phys.mass;arith.ratiodoublenullablee_CARMAGlobSFE? CARMA Global uncertainty on the star formation efficiency (CARMA_Err_Glob_SFE)yr**-1stat.paramdoublenullablee_ACAGlobFco? ACA Global uncertainty on the CO flux (ACA_Err_Glob_Fco)Jy.km.s**-1.beam**-1phot.fluxdoublenullablee_ACAGlobLco? ACA Global uncertainty on the CO luminosity (ACA_Err_Glob_Lco)pc**2.K.km.s**-1phys.luminositydoublenullablee_ACAGlobMmol? ACA Global uncertainty on the molecular gas mass (ACA_Err_Glob_Mmol)solMassphys.massdoublenullablee_ACAGlobfmol? ACA Global uncertainty on the molecular gas mass to stellar mass ratio (ACA_Err_Glob_fmol)phys.mass;arith.ratiodoublenullablee_ACAGlobSFE? ACA Global uncertainty on the star formation efficiency (ACA_Err_Glob_SFE)yr**-1stat.paramdoublenullablee_FinalGlobMmol? Global uncertainty on the molecular gas mass from the consolidated sample (Final_Err_Glob_Mmol)solMassphys.massdoublenullablee_FinalGlobfmol? Global uncertainty on the molecular gas fraction from the consolidated sample (Final_Err_Glob_fmol)phys.mass;arith.ratiodoublenullablee_FinalGlobSFE? Global uncertainty on the star formation efficiency from the consolidated sample (Final_Err_Glob_SFE)yr**-1stat.paramdoublenullableGlobL12W3-7.5? Global 12um luminosity from WISE W3 at 7.5 arcsec resolution (Glob_L12um_w3_7p5)solLumphys.luminositydoublenullablee_GlobL12W3-7.5? Global uncertainty on the 12um luminosity from WISE W3 at 7.5 arcsec resolution (Err_Glob_L12um_w3_7p5)solLumphys.luminositydoublenullableBeamMstarBeam stellar mass (Beam_Mstar)solMassphys.massdoubleBeamSFRBeam star formation rate derived using Balmer decrement (.yr-1 Beam_SFR)solMass/yrphys.SFR;instr.beamdoubleBeamsSFR? Beam specific star formation rate (Beam_sSFR)yr**-1phys.SFR;instr.beamdoublenullablee_BeamMstarBeam uncertainty on the stellar mass (Err_Beam_Mstar)solMassphys.massdoublee_BeamSFRBeam uncertainty on the star formation rate derived using Balmer decrement (Err_Beam_SFR)solMass/yrstat.errordoublee_BeamsSFR? Beam uncertainty on the specific star formation rate (Err_Beam_sSFR)yr**-1stat.errordoublenullableBeamGasMetBeam gas-phase metallicity derived via the O3N2 method (Beam_Gas_Met)phys.abund.ZdoubleBeamaco10b13Beam CO(1-0)-to-H2 conversion factor (Beam_alpha_co10_b13) (1)solMass.K**-1.km**-1.s.pc**-2arith.factordoubleBeamR21Beam CO(2-1)/CO(1-0) flux ratio derived from the star formation rate surface density (Beam_R21)phot.flux;arith.ratiodoubleAPEXBeamk2jyb? APEX Beam Jy/beam per Kelvin (APEX_Beam_k2jypb)J.K**-1.beam**-1arith.factordoublenullableAPEXBeametamb? APEX Beam main beam efficiency (APEX_Beam_eta_mb)stat.paramdoublenullableAPEXBeamTpeak? APEX Beam peak Tmb across the CO spectrum (APEX_Beam_Tpeak)Kphys.temperaturedoublenullableAPEXBeamSNR? APEX Beam signal-to-noise ratio of the CO observation (APEX_Beam_SNR)pos.angDistance;obsdoublenullableAPEXBeamW50m2? APEX Beam full-width half maximum of the CO spectrum calculated via moment 2nd (APEX_Beam_W50_mom2)km/sspect.line.widthdoublenullableAPEXBeamepsob? Beam statistical error for the CO flux (APEX_Beam_eps_obs)K.km/sstat.error;phot.flux;instr.beamdoublenullableAPEXBeamFco? APEX Beam CO flux (APEX_Beam_Fco)Jy.km.s**-1.beam**-1phot.fluxdoublenullableAPEXBeamLco? APEX Beam CO luminosity (APEX_Beam_Lco)pc**2.K.km.s**-1phys.luminositydoublenullableAPEXBeamMmol? APEX Beam molecular gas mass (APEX_Beam_Mmol)solMassphys.massdoublenullableAPEXBeamfmol? APEX Beam molecular gas mass to stellar mass ratio (APEX_Beam_fmol)phys.mass;arith.ratiodoublenullableAPEXBeamSFE? APEX Beam star formation efficiency (APEX_Beam_SFE)yr**-1stat.paramdoublenullableCARMABeamk2jyb? CARMA Beam Jy/beam per Kelvin (CARMA_Beam_k2jypb)Jy.K**-1.beam**-1arith.factordoublenullableCARMABeametamb[-999] CARMA Beam main beam efficiency (CARMA_Beam_eta_mb)stat.paramfloatCARMABeamRMS? CARMA Beam CO noise level (standard deviation of CO spectrum, sigmaRMS) (CARMA_Beam_RMS)Kinstr.det.noise;instr.beamdoublenullableCARMABeamTpeak? CARMA Beam peak Tmb across the CO spectrum (CARMA_Beam_Tpeak)Kphys.temperaturedoublenullableCARMABeamSNR? CARMA Beam signal-to-noise ratio of the CO observation (CARMA_Beam_SNR)pos.angDistance;obsdoublenullableCARMABeamW50m2? CARMA Beam full-width half maximum of the CO spectrum calculated via moment 2nd (CARMA_Beam_W50_mom2)km/sspect.line.widthdoublenullableCARMABeamepsobs?=-999CARMA Beam statistical error for the CO flux (CARMA_Beam_eps_obs)K.km/sstat.error;phot.flux;instr.beamdoubleCARMABeamFco? CARMA Beam CO flux (CARMA_Beam_Fco)Jy.km.s**-1.beam**-1phot.fluxdoublenullableCARMABeamLco? CARMA Beam CO luminosity (CARMA_Beam_Lco)pc**2.K.km.s**-1phys.luminositydoublenullableCARMABeamMmol? CARMA Beam molecular gas mass (CARMA_Beam_Mmol)solMassphys.massdoublenullableCARMABeamfmol? CARMA Beam molecular gas mass to stellar mass ratio (CARMA_Beam_fmol)phys.mass;arith.ratiodoublenullableCARMABeamSFE? CARMA Beam star formation efficiency (CARMA_Beam_SFE)yr**-1stat.paramdoublenullableACABeamk2jyb? ACA Beam Jy/beam per Kelvin (ACA_Beam_k2jypb)Jy.K**-1.beam**-1arith.factordoublenullableACABeametamb[-999] ACA Beam main beam efficiency (ACA_Beam_eta_mb)stat.paramfloatACABeamRMS? ACA Beam CO noise level (standard deviation of CO spectrum, sigmaRMS) (ACA_Beam_RMS)Kinstr.det.noise;instr.beamdoublenullableACABeamTpeak? ACA Beam peak Tmb across the CO spectrum (ACA_Beam_Tpeak)Kphys.temperaturedoublenullableACABeamSNR? ACA Beam signal-to-noise ratio of the CO observation (ACA_Beam_SNR)pos.angDistance;obsdoublenullableACABeamFco? ACA Beam CO flux (ACA_Beam_Fco)Jy.km.s**-1.beam**-1phot.fluxdoublenullableACABeamLco? ACA Beam CO luminosity (ACA_Beam_Lco)pc**2.K.km.s**-1phys.luminositydoublenullableACABeamMmol? ACA Beam molecular gas mass (ACA_Beam_Mmol)solMassphys.massdoublenullableACABeamfmol? ACA Beam molecular gas mass to stellar mass ratio (ACA_Beam_fmol)phys.mass;arith.ratiodoublenullableACABeamSFE? ACA Beam star formation efficiency (ACA_Beam_SFE)yr**-1stat.paramdoublenullableFinalBeamSNRBeam signal-to- noise ratio of the CO observation from the consolidated sample (Final_Beam_SNR)stat.snrdoubleFinalBeamMmolBeam molecular gas mass from the consolidated sample (Final_Beam_Mmol)solMassphys.massdoubleFinalBeamfmol? Beam molecular gas mass fraction from the consolidated sample (Final_Beam_fmol)phys.mass;arith.ratiodoublenullableFinalBeamSFEBeam star formation efficiency from the consolidated sample (Final_Beam_SFE)yr**-1stat.paramdoublee_APEXBeamFco? APEX Beam uncertainty on the CO flux (APEX_Err_Beam_Fco)Jy.km.s**-1.beam**-1phot.fluxdoublenullablee_APEXBeamLco? APEX Beam uncertainty on the CO luminosity (APEX_Err_Beam_Lco)pc**2.K.km.s**-1phys.luminositydoublenullablee_APEXBeamMmol? APEX Beam uncertainty on the molecular gas mass (APEX_Err_Beam_Mmol)solMassphys.massdoublenullablee_APEXBeamfmol? APEX Beam uncertainty on the molecular gas mass to stellar mass ratio (APEX_Err_Beam_fmol)phys.mass;arith.ratiodoublenullablee_APEXBeamSFE? APEX Beam uncertainty on the star formation efficiency (APEX_Err_Beam_SFE)yr**-1stat.paramdoublenullablee_CARMABeamFco? CARMA Beam uncertainty on the CO flux (CARMA_Err_Beam_Fco)Jy.km.s**-1.beam**-1phot.fluxdoublenullablee_CARMABeamLco? CARMA Beam uncertainty on the CO luminosity (CARMA_Err_Beam_Lco)pc**2.K.km.s**-1phys.luminositydoublenullablee_CARMABeamMmol? CARMA Beam uncertainty on the molecular gas mass (CARMA_Err_Beam_Mmol)solMassphys.massdoublenullablee_CARMABeamfmol? CARMA Beam uncertainty on the molecular gas mass to stellar mass ratio (CARMA_Err_Beam_fmol)phys.mass;arith.ratiodoublenullablee_CARMABeamSFE? CARMA Beam uncertainty on the star formation efficiency (CARMA_Err_Beam_SFE)yr**-1stat.paramdoublenullablee_ACABeamFco? ACA Beam uncertainty on the CO flux (ACA_Err_Beam_Fco)Jy.km.s**-1.beam**-1phot.fluxdoublenullablee_ACABeamLco? ACA Beam uncertainty on the CO luminosity (ACA_Err_Beam_Lco)pc**2.K.km.s**-1phys.luminositydoublenullablee_ACABeamMmol? ACA Beam uncertainty on the molecular gas mass (ACA_Err_Beam_Mmol)solMassphys.massdoublenullablee_ACABeamfmol? ACA Beam uncertainty on the molecular gas mass to stellar mass ratio (ACA_Err_Beam_fmol)phys.mass;arith.ratiodoublenullablee_ACABeamSFE? ACA Beam uncertainty on the star formation efficiency (ACA_Err_Beam_SFE)yr**-1stat.paramdoublenullablee_FinalBeamMmol? Beam uncertainty on the molecular gas mass from the consolidated sample (Final_Err_Beam_Mmol)solMassphys.massdoublenullablee_FinalBeamfmol? Beam uncertainty on the molecular gas fraction from the consolidated sample (Final_Err_Beam_fmol)phys.mass;arith.ratiodoublenullablee_FinalBeamSFE? Beam uncertainty on the star formation efficiency from the consolidated sample (Final_Err_Beam_SFE)yr**-1stat.paramdoublenullablee_BeamL12W3-7.5? Beam uncertainty on the 12um luminosity from WISE W3 at 7.5 arcsec resolution (Err_Beam_L12um_w3_7p5)solLumphys.luminositydoublenullableMorphologyGalaxy morphology obtained from Hyperleda (Morphology)src.morph.typecharf_FinalQS[1/3] Quenching stage classification quality flag (Final_flag_QS) (4)meta.code.qualintf_FinalNA[SU] Nuclear activity classification quality flag (Final_flag_NA) (5)meta.code.qualcharCALIFAName of the galaxy as indicated in the CALIFA extended DR3 (CALIFA_name)meta.id;meta.maincharFinalGlobObsObservatory of the Global CO measurement included in the consolidated sample (Final_Glob_Observatory)meta.idcharFinalBeamObsObservatory of the Beam CO measurement included in the consolidated sample (Final_Beam_Observatory)meta.idcharCARMAconfCARMA configuration (CARMA_conf)meta.codechar