J/A+A/699/A366 EDGE-CALIFA Survey. iEDGE. (Colombo+, 2025)
The EDGE-CALIFA survey: An integral field unit-based integrated molecular gas
database for galaxy evolution studies in the Local Universe.
Colombo 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.
<Astron. Astrophys. 699, A366 (2025)>
=2025A&A...699A.366C 2025A&A...699A.366C (SIMBAD/NED BibCode)
ADC_Keywords: Galaxy catalogs ; Molecular data ; Equivalent widths ;
Abundances ; Carbon monoxide
Keywords: ISM: molecules - galaxies: evolution - galaxies: ISM -
galaxies: star formation
Abstract:
Studying 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.
Description:
Database of optical and CO integrated quantities for 643 galaxies
observed by CALIFA (eDR3) and a set of mm-telescopes (APEX, CARMA, and
ACA) presented in the paper (Table C.1). Global measurements are
integrated across the full extent of the galaxy disc, while Beam
measurements are obtained within the APEX beam at 230GHz (e.g. within
the inner 26.3 arcsec). In the case that a given source was not
observed with the given facility, the quantity assumes a NaN entry.
Quantities measured from non-detected CO observation (with S/N<3) are
included as upper limits. For the morphology (obtained from
HyperLEDA), we simply separated the galaxies as spiral (S), elliptical
(E), lenticular (S0), and irregular (I), without considering the
sub-classes of spirals (except intermediate spirals, SABs; and barred
spirals, SBs) and elliptical morphologies. Galaxies for which the
morphology is not provided are indicated with 'U'. A galaxy quenching
stage (QS) and nuclear activity (NA) is classified via the QueStNA
scheme based on optical emission line measurements (Kalinova et al.
2021A&A...648A..64K 2021A&A...648A..64K, Cat. J/A+A/648/A64). The quenching stages
considered are: SF -- star-forming, QnR -- quenched-nuclear-ring,
cQ -- centrally-quiescent, MX -- mixed, nR -- nearly- retired, fR --
fully-retired. The nuclear activities considered are: nonA --
non-active, wAGN -- weak AGN host, sAGN -- strong AGN host. The
quality flags on the quenching stage classification considered are:
1 -- sure class, 2 -- unsure class due to median Halpha equivalent
width close to thresholds, 3 -- unsure class due to median Halpha
equivalent width differences between the 1-sigma and 3-sigma
masked data. The quality flags on the nuclear activity classification
considered are: S -- sure class based on the information of the
three BPT diagrams, U -- unsure class based on the information of
two of the three BPT diagrams.
Blank entries are indicated with -999 or "blank".
File Summary:
--------------------------------------------------------------------------------
FileName Lrecl Records Explanations
--------------------------------------------------------------------------------
ReadMe 80 . This file
tablec1.dat 3306 643 Integrated CO and optical measurements for
643 local galaxies
--------------------------------------------------------------------------------
See also:
J/A+A/648/A64 : Star formation quenching stages of galaxies (Kalinova+ 2021)
J/ApJ/846/159 : Interferometric CO obs. of 126 CALIFA galaxies
(Bolatto+, 2017)
J/MNRAS/484/5192 : Molecular gas distribution and star formation (Chown+, 2019)
Byte-by-byte Description of file: tablec1.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 22 A22 --- CALIFA Name of the galaxy as
indicated in the CALIFA
extended DR3 (CALIFA_name)
24- 50 A27 --- OName Alternative name of the
galaxy (Alias)
52- 72 F21.17 deg RAdeg Right ascension of the
galaxy centre (J2000) (RA)
74- 94 F21.17 deg DEdeg Declination of the galaxy
centre (J2000) (DEC)
96- 115 F20.14 km/s Vlsr LSR velocity of the galaxy,
derived from the stellar
redshift (Vlsr)
117- 136 F20.18 --- zstar Stellar redshift of the
galaxy (zstar)
138- 157 F20.16 Mpc Distance Distance to the galaxy
(Distance)
159- 175 F17.14 deg Incl Galaxy inclination (Incl)
177- 193 F17.13 deg PA Galaxy position angle (PA)
195- 212 F18.14 arcsec Re Galaxy effective radius
(Re_as)
214- 232 F19.16 0.1nm GlobmedEWHa Global median Halpha
equivalent width
(GlobmedEWHa)
234- 254 F21.8 Msun GlobMstar Global stellar mass
(Glob_Mstar)
256- 277 E22.22 Msun/yr GlobSFR Global star formation rate
derived using Balmer
decrement (Glob_SFR)
279- 300 E22.17 yr-1 GlobsSFR ?=-999 Global specific star
formation rate (Glob_sSFR)
302- 323 F22.9 Msun e_GlobMstar Global uncertainty on the
stellar mass
(ErrGlobMstar)
325- 346 E22.21 Msun/yr e_GlobSFR Global uncertainty on the
star formation rate
derived using Balmer
decrement (ErrGlobSFR)
348- 369 E22.17 yr-1 e_GlobsSFR ?=-999 Global uncertainty
on the specific star
formation rate
(ErrGlobsSFR)
371- 387 F17.15 --- GlobGasMet Global gas-phase
metallicity derived via
the O3N2 method
(GlobGasMet)
389- 406 F18.16 Msun/(K.(km/s).pc2) Globaco10b13 Global CO(1-0)-to-H2
conversion factor
(Globalphaco10_b13) (1)
408- 425 F18.16 --- GlobR21 Global CO(2-1)/CO(1-0) flux
ratio derived from the
star formation rate
surface density (Glob_R21)
427- 432 F6.1 Jy/K/beam APEXGlobk2jyb [-999] APEX Global Jy/beam
per Kelvin
(APEXGlobk2jypb)
434- 454 F21.16 --- APEXGlobetamb ?=-999 APEX Global main
beam efficiency
(APEXGlobeta_mb)
456- 480 F25.20 K APEXGlobRMS ?=-999 APEX Global CO noise
level (standard deviation
of CO spectrum, sigmaRMS)
(APEXGlobRMS)
482- 505 F24.19 K APEXGlobTpeak ?=-999 APEX Global peak
Tmb across the CO spectrum
(APEXGlobTpeak)
507- 527 F21.16 --- APEXGlobSNR ?=-999 APEX Global
signal-to-noise ratio of
the CO observation
(APEXGlobSNR)
529- 548 F20.15 km/s APEXGlobW50m2 ?=-999 APEX Global
full-width half maximum of
the CO spectrum calculated
via moment 2nd
(APEXGlobW50_mom2)
550- 572 F23.18 K.km/s APEXGlobepsobs ?=-999 APEX Global
statistical error for the
CO flux
(APEXGlobeps_obs)
574- 594 F21.16 Jy.km/s/beam APEXGlobFco ?=-999 APEX Global CO flux
(APEXGlobFco)
596- 618 F23.11 pc2.K.km/s APEXGlobLco ?=-999 APEX Global CO
luminosity (APEXGlobLco)
620- 641 F22.10 Msun APEXGlobMmol ?=-999 APEX Global
molecular gas mass
(APEXGlobMmol)
643- 667 F25.20 --- APEXGlobfmol ?=-999 APEX Global
molecular gas mass to
stellar mass ratio
(APEXGlobfmol)
669- 690 E22.17 yr-1 APEXGlobSFE ?=-999 APEX Global star
formation efficiency
(APEXGlobSFE)
692- 713 F22.17 Jy/K/beam CARMAGlobk2jyb ?=-999 CARMA Global Jy/beam
per Kelvin
(CARMAGlobk2jypb)
715- 720 F6.1 --- CARMAGlobetamb [-999] CARMA Global main
beam efficiency
(CARMAGlobeta_mb)
722- 744 F23.18 K CARMAGlobRMS ?=-999 CARMA Global CO
noise level (standard
deviation of CO spectrum,
sigmaRMS) (CARMAGlobRMS)
746- 767 F22.17 K CARMAGlobTpeak ?=-999 CARMA Global peak
Tmb across the CO spectrum
(CARMAGlobTpeak)
769- 775 F7.2 --- CARMAGlobSNR ?=-999 CARMA Global
signal-to-noise ratio of
the CO observation
(CARMAGlobSNR)
777- 796 F20.15 km/s CARMAGlobW50m2 ?=-999 CARMA Global
full-width half maximum of
the CO spectrum calculated
via moment 2nd
(CARMAGlobW50_mom2)
798- 816 F19.14 K.km/s CARMAGlobepsob ?=-999 CARMA Global
statistical error for the
CO flux
(CARMAGlobeps_obs)
818- 824 F7.2 Jy.km/s/beam CARMAGlobFco ?=-999 CARMA Global CO flux
(CARMAGlobFco)
826- 845 F20.9 pc2.K.km/s CARMAGlobLco ?=-999 CARMA Global CO
luminosity
(CARMAGlobLco)
847- 866 F20.8 Msun CARMAGlobMmol ?=-999 CARMA Global
molecular gas mass
(CARMAGlobMmol)
868- 891 F24.19 --- CARMAGlobfmol ?=-999 CARMA Global
molecular gas mass to
stellar mass ratio
(CARMAGlobfmol)
893- 914 E22.17 yr-1 CARMAGlobSFE ?=-999 CARMA Global star
formation efficiency
(CARMAGlobSFE)
916- 937 F22.17 Jy/K/beam ACAGlobk2jyb ?=-999 ACA Global Jy/beam
per Kelvin
(ACAGlobk2jypb)
939- 944 F6.1 --- ACAGlobetamb [-999] ACA Global main beam
efficiency
(ACAGlobeta_mb)
946- 968 F23.18 K ACAGlobRMS ?=-999 ACA Global CO noise
level (standard deviation
of CO spectrum, sigmaRMS)
(ACAGlobRMS)
970- 992 F23.18 K ACAGlobTpeak ?=-999 ACA Global peak Tmb
across the CO spectrum
(ACAGlobTpeak)
994-1014 F21.16 --- ACAGlobSNR ?=-999 ACA Global
signal-to-noise ratio of
the CO observation
(ACAGlobSNR)
1016-1034 F19.14 km/s ACAGlobW50m2 ?=-999 ACA Global
full-width half maximum of
the CO spectrum calculated
via moment 2nd
(ACAGlobW50_mom2)
1036-1055 F20.14 K.km/s ACAGlobepsob ?=-999 ACA Global
statistical error for the
CO flux (ACAGlobeps_obs)
1057-1077 F21.16 Jy.km/s/beam ACAGlobFco ?=-999 ACA Global CO flux
(ACAGlobFco)
1079-1098 F20.9 pc2.K.km/s ACAGlobLco ?=-999 ACA Global CO
luminosity (ACAGlobLco)
1100-1119 F20.9 Msun ACAGlobMmol ?=-999 ACA Global molecular
gas mass (ACAGlobMmol)
1121-1144 F24.19 --- ACAGlobfmol ?=-999 ACA Global molecular
gas mass to stellar mass
ratio (ACAGlobfmol)
1146-1167 E22.17 yr-1 ACAGlobSFE ?=-999 ACA Global star
formation efficiency
(ACAGlobSFE)
1169-1173 A5 --- FinalGlobObs Observatory of the Global
CO measurement included in
the consolidated sample
(FinalGlobObservatory)
1175-1194 F20.16 --- FinalGlobSNR Global signal-to-noise
ratio of the CO
observation from the
consolidated sample
(FinalGlobSNR)
1196-1217 F22.10 Msun FinalGlobMmol Global molecular gas mass
from the consolidated
sample (FinalGlobMmol)
1219-1243 F25.20 --- FinalGlobfmol ?=-999 Global molecular gas
mass fraction from the
consolidated sample
(FinalGlobfmol)
1245-1266 E22.17 yr-1 FinalGlobSFE Global star formation
efficiency from the
consolidated sample
(FinalGlobSFE)
1268-1288 F21.16 Jy.km/s/beam e_APEXGlobFco ?=-999 APEX Global
uncertainty on the CO flux
(APEXErrGlob_Fco)
1290-1311 F22.12 pc2.K.km/s e_APEXGlobLco ?=-999 APEX Global
uncertainty on the CO
luminosity
(APEXErrGlob_Lco)
1313-1332 F20.10 Msun e_APEXGlobMmol ?=-999 APEX Global
uncertainty on the
molecular gas mass
(APEXErrGlob_Mmol)
1334-1358 F25.20 --- e_APEXGlobfmol ?=-999 APEX Global
uncertainty on the
molecular gas mass to
stellar mass ratio
(APEXErrGlob_fmol)
1360-1381 E22.17 yr-1 e_APEXGlobSFE ?=-999 APEX Global
uncertainty on the star
formation efficiency
(APEXErrGlob_SFE)
1383-1403 F21.16 Jy.km/s/beam e_CARMAGlobFco ?=-999 CARMA Global
uncertainty on the CO flux
(CARMAErrGlob_Fco)
1405-1424 F20.10 pc2.K.km/s e_CARMAGlobLco ?=-999 CARMA Global
uncertainty on the CO
luminosity
(CARMAErrGlob_Lco)
1426-1444 F19.9 Msun e_CARMAGlobMmol ?=-999 CARMA Global
uncertainty on the
molecular gas mass
(CARMAErrGlob_Mmol)
1446-1470 F25.19 --- e_CARMAGlobfmol ?=-999 CARMA Global
uncertainty on the
molecular gas mass to
stellar mass ratio
(CARMAErrGlob_fmol)
1472-1493 E22.17 yr-1 e_CARMAGlobSFE ?=-999 CARMA Global
uncertainty on the star
formation efficiency
(CARMAErrGlob_SFE)
1495-1515 F21.16 Jy.km/s/beam e_ACAGlobFco ?=-999 ACA Global
uncertainty on the CO flux
(ACAErrGlob_Fco)
1517-1535 F19.9 pc2.K.km/s e_ACAGlobLco ?=-999 ACA Global
uncertainty on the CO
luminosity
(ACAErrGlob_Lco)
1537-1556 F20.9 Msun e_ACAGlobMmol ?=-999 ACA Global
uncertainty on the
molecular gas mass
(ACAErrGlob_Mmol)
1558-1583 F26.20 --- e_ACAGlobfmol ?=-999 ACA Global
uncertainty on the
molecular gas mass to
stellar mass ratio
(ACAErrGlob_fmol)
1585-1606 E22.17 yr-1 e_ACAGlobSFE ?=-999 ACA Global
uncertainty on the star
formation efficiency
(ACAErrGlob_SFE)
1608-1628 F21.10 Msun e_FinalGlobMmol ?=-999 Global uncertainty
on the molecular gas mass
from the consolidated
sample
(FinalErrGlob_Mmol)
1630-1654 F25.20 --- e_FinalGlobfmol ?=-999 Global uncertainty
on the molecular gas
fraction from the
consolidated sample
(FinalErrGlob_fmol)
1656-1677 E22.17 yr-1 e_FinalGlobSFE ?=-999 Global uncertainty
on the star formation
efficiency from the
consolidated sample
(FinalErrGlob_SFE)
1679-1701 F23.11 Lsun GlobL12W3-7.5 ?=-999 Global 12um
luminosity from WISE W3 at
7.5 arcsec resolution
(GlobL12umw3_7p5)
1703-1723 F21.11 Lsun e_GlobL12W3-7.5 ?=-999 Global uncertainty
on the 12um luminosity
from WISE W3 at 7.5 arcsec
resolution
(ErrGlobL12umw37p5)
1725-1743 F19.16 0.1nm BeammedEWHa Beam median Halpha
equivalent width
(BeammedEWHa)
1745-1766 F22.9 Msun BeamMstar Beam stellar mass
(Beam_Mstar)
1768-1789 E22.22 Msun/yr BeamSFR Beam star formation rate
derived using Balmer
decrement (.yr-1 Beam_SFR)
1791-1812 E22.17 yr-1 BeamsSFR ?=-999 Beam specific star
formation rate (Beam_sSFR)
1814-1834 F21.9 Msun e_BeamMstar Beam uncertainty on the
stellar mass
(ErrBeamMstar)
1836-1857 E22.21 Msun/yr e_BeamSFR Beam uncertainty on the
star formation rate
derived using Balmer
decrement (ErrBeamSFR)
1859-1880 E22.17 yr-1 e_BeamsSFR ?=-999 Beam uncertainty on
the specific star
formation rate
(ErrBeamsSFR)
1882-1898 F17.15 --- BeamGasMet Beam gas-phase metallicity
derived via the O3N2
method (BeamGasMet)
1900-1918 F19.16 Msun/(K.(km/s).pc2) Beamaco10b13 Beam CO(1-0)-to-H2
conversion factor
(Beamalphaco10_b13) (1)
1920-1937 F18.16 --- BeamR21 Beam CO(2-1)/CO(1-0) flux
ratio derived from the
star formation rate
surface density (Beam_R21)
1939-1958 F20.15 J/K/beam APEXBeamk2jyb ?=-999 APEX Beam Jy/beam
per Kelvin
(APEXBeamk2jypb)
1960-1980 F21.16 --- APEXBeametamb ?=-999 APEX Beam main beam
efficiency
(APEXBeameta_mb)
1982-2006 F25.20 K APEXBeamRMS ?=-999 APEX Beam CO noise
level (standard deviation
of CO spectrum, sigmaRMS)
(APEXBeamRMS)
2008-2031 F24.19 K APEXBeamTpeak ?=-999 APEX Beam peak Tmb
across the CO spectrum
(APEXBeamTpeak)
2033-2053 F21.16 --- APEXBeamSNR ?=-999 APEX Beam
signal-to-noise ratio of
the CO observation
(APEXBeamSNR)
2055-2074 F20.15 km/s APEXBeamW50m2 ?=-999 APEX Beam full-width
half maximum of the CO
spectrum calculated via
moment 2nd
(APEXBeamW50_mom2)
2076-2098 F23.18 K.km/s APEXBeamepsob ?=-999 Beam statistical
error for the CO flux
(APEXBeameps_obs)
2100-2120 F21.16 Jy.km/s/beam APEXBeamFco ?=-999 APEX Beam CO flux
(APEXBeamFco)
2122-2143 F22.11 pc2.K.km/s APEXBeamLco ?=-999 APEX Beam CO
luminosity (APEXBeamLco)
2145-2166 F22.10 Msun APEXBeamMmol ?=-999 APEX Beam molecular
gas mass (APEXBeamMmol)
2168-2192 F25.20 --- APEXBeamfmol ?=-999 APEX Beam molecular
gas mass to stellar mass
ratio (APEXBeamfmol)
2194-2215 E22.17 yr-1 APEXBeamSFE ?=-999 APEX Beam star
formation efficiency
(APEXBeamSFE)
2217-2235 F19.14 Jy/K/beam CARMABeamk2jyb ?=-999 CARMA Beam Jy/beam
per Kelvin
(CARMABeamk2jypb)
2237-2242 F6.1 --- CARMABeametamb [-999] CARMA Beam main beam
efficiency
(CARMABeameta_mb)
2244-2267 F24.19 K CARMABeamRMS ?=-999 CARMA Beam CO noise
level (standard deviation
of CO spectrum, sigmaRMS)
(CARMABeamRMS)
2269-2292 F24.19 K CARMABeamTpeak ?=-999 CARMA Beam peak Tmb
across the CO spectrum
(CARMABeamTpeak)
2294-2314 F21.16 --- CARMABeamSNR ?=-999 CARMA Beam
signal-to-noise ratio of
the CO observation
(CARMABeamSNR)
2316-2335 F20.15 km/s CARMABeamW50m2 ?=-999 CARMA Beam
full-width half maximum of
the CO spectrum calculated
via moment 2nd
(CARMABeamW50_mom2)
2337-2359 F23.18 K.km/s CARMABeamepsobs?=-999 CARMA Beam
statistical error for the
CO flux
(CARMABeameps_obs)
2361-2381 F21.16 Jy.km/s/beam CARMABeamFco ?=-999 CARMA Beam CO flux
(CARMABeamFco)
2383-2402 F20.9 pc2.K.km/s CARMABeamLco ?=-999 CARMA Beam CO
luminosity
(CARMABeamLco)
2404-2424 F21.9 Msun CARMABeamMmol ?=-999 CARMA Beam molecular
gas mass (CARMABeamMmol)
2426-2449 F24.19 --- CARMABeamfmol ?=-999 CARMA Beam molecular
gas mass to stellar mass
ratio (CARMABeamfmol)
2451-2472 E22.17 yr-1 CARMABeamSFE ?=-999 CARMA Beam star
formation efficiency
(CARMABeamSFE)
2474-2493 F20.15 Jy/K/beam ACABeamk2jyb ?=-999 ACA Beam Jy/beam per
Kelvin (ACABeamk2jypb)
2495-2500 F6.1 --- ACABeametamb [-999] ACA Beam main beam
efficiency
(ACABeameta_mb)
2502-2523 E22.17 K ACABeamRMS ?=-999 ACA Beam CO noise
level (standard deviation
of CO spectrum, sigmaRMS)
(ACABeamRMS)
2525-2549 F25.20 K ACABeamTpeak ?=-999 ACA Beam peak Tmb
across the CO spectrum
(ACABeamTpeak)
2551-2571 F21.16 --- ACABeamSNR ?=-999 ACA Beam
signal-to-noise ratio of
the CO observation
(ACABeamSNR)
2573-2591 F19.14 km/s ACABeamW50m2 ?=-999 ACA Beam full- width
half maximum of the CO
spectrum calculated via
moment 2nd
(ACABeamW50_mom2)
2593-2616 F24.19 K.km/s ACABeamepsobs ?=-999 ACA Beam statistical
error for the CO flux
(ACABeameps_obs)
2618-2638 F21.16 Jy.km/s/beam ACABeamFco ?=-999 ACA Beam CO flux
(ACABeamFco)
2640-2659 F20.10 pc2.K.km/s ACABeamLco ?=-999 ACA Beam CO
luminosity (ACABeamLco)
2661-2681 F21.10 Msun ACABeamMmol ?=-999 ACA Beam molecular
gas mass (ACABeamMmol)
2683-2707 F25.20 --- ACABeamfmol ?=-999 ACA Beam molecular
gas mass to stellar mass
ratio (ACABeamfmol)
2709-2730 E22.17 yr-1 ACABeamSFE ?=-999 ACA Beam star
formation efficiency
(ACABeamSFE)
2732-2736 A5 --- FinalBeamObs Observatory of the Beam CO
measurement included in
the consolidated sample
(FinalBeamObservatory)
2738-2758 F21.16 --- FinalBeamSNR Beam signal-to- noise ratio
of the CO observation from
the consolidated sample
(FinalBeamSNR)
2760-2781 F22.10 Msun FinalBeamMmol Beam molecular gas mass
from the consolidated
sample (FinalBeamMmol)
2783-2807 F25.20 --- FinalBeamfmol ?=-999 Beam molecular gas
mass fraction from the
consolidated sample
(FinalBeamfmol)
2809-2830 E22.17 yr-1 FinalBeamSFE Beam star formation
efficiency from the
consolidated sample
(FinalBeamSFE)
2832-2852 F21.16 Jy.km/s/beam e_APEXBeamFco ?=-999 APEX Beam
uncertainty on the CO flux
(APEXErrBeam_Fco)
2854-2875 F22.12 pc2.K.km/s e_APEXBeamLco ?=-999 APEX Beam
uncertainty on the CO
luminosity
(APEXErrBeam_Lco)
2877-2896 F20.10 Msun e_APEXBeamMmol ?=-999 APEX Beam
uncertainty on the
molecular gas mass
(APEXErrBeam_Mmol)
2898-2921 F24.19 --- e_APEXBeamfmol ?=-999 APEX Beam
uncertainty on the
molecular gas mass to
stellar mass ratio
(APEXErrBeam_fmol)
2923-2944 E22.17 yr-1 e_APEXBeamSFE ?=-999 APEX Beam
uncertainty on the star
formation efficiency
(APEXErrBeam_SFE)
2946-2967 F22.17 Jy.km/s/beam e_CARMABeamFco ?=-999 CARMA Beam
uncertainty on the CO flux
(CARMAErrBeam_Fco)
2969-2987 F19.10 pc2.K.km/s e_CARMABeamLco ?=-999 CARMA Beam
uncertainty on the CO
luminosity
(CARMAErrBeam_Lco)
2989-3008 F20.10 Msun e_CARMABeamMmol ?=-999 CARMA Beam
uncertainty on the
molecular gas mass
(CARMAErrBeam_Mmol)
3010-3034 F25.20 --- e_CARMABeamfmol ?=-999 CARMA Beam
uncertainty on the
molecular gas mass to
stellar mass ratio
(CARMAErrBeam_fmol)
3036-3057 E22.17 yr-1 e_CARMABeamSFE ?=-999 CARMA Beam
uncertainty on the star
formation efficiency
(CARMAErrBeam_SFE)
3059-3080 F22.17 Jy.km/s/beam e_ACABeamFco ?=-999 ACA Beam uncertainty
on the CO flux
(ACAErrBeam_Fco)
3082-3101 F20.11 pc2.K.km/s e_ACABeamLco ?=-999 ACA Beam uncertainty
on the CO luminosity
(ACAErrBeam_Lco)
3103-3122 F20.11 Msun e_ACABeamMmol ?=-999 ACA Beam uncertainty
on the molecular gas mass
(ACAErrBeam_Mmol)
3124-3145 E22.17 --- e_ACABeamfmol ?=-999 ACA Beam uncertainty
on the molecular gas mass
to stellar mass ratio
(ACAErrBeam_fmol)
3147-3168 E22.17 yr-1 e_ACABeamSFE ?=-999 ACA Beam uncertainty
on the star formation
efficiency
(ACAErrBeam_SFE)
3170-3190 F21.11 Msun e_FinalBeamMmol ?=-999 Beam uncertainty on
the molecular gas mass
from the consolidated
sample
(FinalErrBeam_Mmol)
3192-3213 E22.17 --- e_FinalBeamfmol ?=-999 Beam uncertainty on
the molecular gas fraction
from the consolidated
sample
(FinalErrBeam_fmol)
3215-3236 E22.17 yr-1 e_FinalBeamSFE ?=-999 Beam uncertainty on
the star formation
efficiency from the
consolidated sample
(FinalErrBeam_SFE)
3238-3261 F24.12 Lsun BeamL12W3-7.5 ?=-999 Beam 12um luminosity
from WISE W3 at 7.5 arcsec
resolution
(BeamL12umw3_7p5)
3263-3283 F21.11 Lsun e_BeamL12W3-7.5 ?=-999 Beam uncertainty on
the 12um luminosity from
WISE W3 at 7.5 arcsec
resolution
(ErrBeamL12umw37p5)
3285-3288 A4 --- CARMAconf CARMA configuration
(CARMA_conf)
3290-3293 A4 --- Morphology Galaxy morphology obtained
from Hyperleda
(Morphology)
3295-3297 A3 --- FinalQS Quenching stage
classification
(Final_QS) (2)
3299-3302 A4 --- FinalNA Nuclear activity
classification
(Final_NA) (3)
3304 I1 --- f_FinalQS [1/3] Quenching stage
classification quality
flag (FinalflagQS) (4)
3306 A1 --- f_FinalNA [SU] Nuclear activity
classification quality
flag (FinalflagNA) (5)
--------------------------------------------------------------------------------
Note (1): derived following Bolatto et al. (2013ARA&A..51..207B 2013ARA&A..51..207B)
(in Msun/(K.(km/s).pc2) units).
Note (2): Quenching stage classification as follows:
MX = mixed
QnR = quenched-nuclear-ring
SF = star-forming
cQ = centrally-quiescent
fR = fully-retired
nR = nearly- retired
Note (3): Nuclear activity classification as follows:
nonA = non-active
sAGN = strong AGN host
wAGN = weak AGN host
Note (4): Quality flags on the quenching stage classification as follows:
1 = sure class
2 = unsure class due to median Halpha equivalent width close to thresholds
3 = unsure class due to median Halpha equivalent width differences between
the 1-sigma and 3-sigma masked data
Note (5): Quality flags on the nuclear activity classification as follows:
S = sure class based on the information of the three BPT diagrams
U = unsure class based on the information of two of the three BPT diagrams
--------------------------------------------------------------------------------
Acknowledgements:
Dario Colombo, dcolombo(at)uni-bonn.de
References:
Bolatto et al., 2017ApJ...846..159B 2017ApJ...846..159B, Cat. J/ApJ/846/159
Utomo et al., 2017ApJ...849...26U 2017ApJ...849...26U
Levy et al., 2018ApJ...860...92L 2018ApJ...860...92L
Colombo et al., 2018MNRAS.475.1791C 2018MNRAS.475.1791C
Leung et al., 2018MNRAS.477..254L 2018MNRAS.477..254L
Levy et al., 2019ApJ...882...84L 2019ApJ...882...84L
Dey et al., 2019MNRAS.488.1926D 2019MNRAS.488.1926D
Colombo et al., 2020A&A...644A..97C 2020A&A...644A..97C
Barrera-Ballesteros et al., 2020MNRAS.492.2651B 2020MNRAS.492.2651B
Villanueva et al., 2021ApJ...923...60V 2021ApJ...923...60V
Sanchez et al. 2021MNRAS.503.1615S 2021MNRAS.503.1615S
Barrera-Ballesteros et al., 2021MNRAS.503.3643B 2021MNRAS.503.3643B
Ellison et al., 2021MNRAS.505L..46E 2021MNRAS.505L..46E
Yu et al. 2022A&A...666A.175Y 2022A&A...666A.175Y
Cao et al., 2023ApJS..268....3C 2023ApJS..268....3C
Villanueva et al., 2024ApJ...962...88V 2024ApJ...962...88V
Wong et al., 2024ApJS..271...35W 2024ApJS..271...35W
Bazzi et al., 2025A&A...697A.149B 2025A&A...697A.149B
(End) Patricia Vannier [CDS] 13-Jun-2025