J/A+A/702/A187 GLACE survey: The mass--SFR relation (De Daniloff+, 2025)
GLACE survey: OSIRIS/GTC multi-object spectroscopy of the rich galaxy cluster
ZwCl 0024.0+1652 at z∼0.4.
III. The mass-SFR relation and the quenching of cluster galaxies.
De Daniloff S.B., Bongiovanni A., Sanchez-Portal M., Cedres B.,
Padilla-Torres C.P., Perez-Garcia A.M., Perez-Martinez R., Espada D.,
de la Casa C.C., Torres-Rios G., Gonzalez-Otero M., de Diego J.A.,
Rodriguez M.I., Cervino M., Lara-Lopez M.A., Cepa J., Valtchanov I.,
Gonzalez-Serrano J.I., Cruz-Gonzalez I., Negrete C.A., Beyoro-Amado Z.,
Castillo-Fraile M., Mancillas B., Povic M.
<Astron. Astrophys. 702, A187 (2025)>
=2025A&A...702A.187D 2025A&A...702A.187D (SIMBAD/NED BibCode)
ADC_Keywords: Galaxies, optical ; Galaxy catalogs ; Spectroscopy ; Photometry ;
Models, evolutionary
Keywords: techniques: spectroscopic - galaxies: abundances - galaxies: active -
galaxies: distances and redshifts -
galaxies: clusters: individual: ZwCl 0024.0+1652 -
galaxies: star formation
Abstract:
Galaxy clusters are among the largest and densest structures in the
Universe. Their high density generally increases the suppression of
star formation, known as quenching, altering galaxy properties.
We study the quenching of emission-line galaxies (ELGs) in the rich
cluster ZwCl 0024.0+1652 (Cl0024) at redshift z∼0.4, aiming to
determine if and how star formation is suppressed.
Using multi-object spectroscopy from the GLACE survey, we extract
fluxes and redshifts of [OII]3727,3729, Hbeta, and [OIII]5007 emission
lines to derive star formation rates (SFRs) for 173 ELGs. We also
perform spectral energy distribution fitting to obtain key
evolutionary parameters such as stellar masses and the 4000 Angstrom
break (D4000) index.
We derive the stellar mass-SFR relation for 98 star-forming galaxies,
finding 34.7% exhibit suppressed SFRs in the cluster, compared to
11.0% in the field. While SFRs show no significant variation with
local density, the fraction of SFGs is 1.55 times higher in the
cluster outskirts than in intermediate-density regions. The specific
SFR decreases strongly with $D4000$ for active SFGs but remains
constant for suppressed galaxies. The fraction of suppressed galaxies
in the infall region is 2.6 times higher than in the core, and
especially in the infalling structure B of the cluster. The
cluster's total mass does not appear to be a key factor in SFG
quenching.
Star formation in Cl0024 galaxies is suppressed by the dense cluster
environment. This suppression is evident in SFG fractions and
parameters tracing long-term evolution, indicating prolonged
quenching. SFGs preferentially reside in low-density regions, while
suppressed galaxies dominate the infall region, supporting a
"delayed-then-rapid" quenching scenario.
Description:
We present a catalogue of physical properties for 101 star-forming
galaxies of the galaxy cluster ZwCl 0024.0+1652, selected from the
GLACE survey.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
catalog.dat 3288 102 Catalog of the properties of the galaxies
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See also:
J/MNRAS/501/2430 : Galaxy activity in ZwCl0024+1652 cluster
(Beyoro-Amado+, 2021)
Byte-by-byte Description of file: catalog.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 7 A7 --- ID-unique GLACE ID with pointing label,
NNNNN_a (id_unique) (1)(2)
9- 13 I5 --- ID GLACE ID without pointing label
(ID) (1)
15- 19 A5 --- ID-MOS ID of the MOS spectrum after
reduction (id_MOS)
21- 29 F9.7 deg RAdeg Right ascension (J2000) from TF
(tunable filters) calibrated data
(RA_J2000) (1)
31- 40 F10.7 deg DEdeg Declination (J2000) from TF
calibrated data (DEC_J2000) (1)
42- 49 F8.6 deg RAGdeg Right ascension from GAIA-DR1
(ICRS) at Ep=2015.0 (RA_GAIA) (1)
51- 58 F8.5 deg DEGdeg Declination from GAIA- DR1 (ICRS)
at Ep=2015.0 (DEC_GAIA) (1)
60- 67 F8.6 --- zSP15 Redshift from TF calibrated data
(Sanchez-Portal et al.,
2015A&A...578A..30S 2015A&A...578A..30S,) (z_SP15)
69- 76 F8.6 --- zHaIC Redshift of Halpha emission line
obtained from inverse convolution
method (zHalphaInvConv) (3)
78- 85 F8.6 --- b_zHaIC Lower value of redshift of Halpha
emission line
(zHalphaInvConv_d) (3)
87- 94 F8.6 --- B_zHaIC Upper value of redshift of Halpha
emission line
(zHalphaInvConv_u) (3)
96- 114 F19.17 --- zOII ? Redshift of [OII] emission
line (z_OII)
116- 137 F22.20 --- e_zOII ? Error in redshift of [OII]
emission line (ezOII)
139- 157 F19.17 --- zHb ? Redshift of Hbeta emission line
(z_Hbeta)
159- 180 F22.20 --- e_zHb ? Error in redshift of Hbeta
emission line (ezHbeta)
182- 200 F19.17 --- zOIII ? Redshift of [OIII]5007 emission
line (z_OIII)
202- 223 F22.20 --- e_zOIII ? Error in redshift of [OIII]5007
emission line (ezOIII)
225- 243 F19.17 --- zMOSavg ? Average redshift of [OII],
Hbeta, and [OIII]5007 emission
lines (zMOSavg)
245- 266 F22.20 --- e_zMOSavg ? Error in average redshift of
[OII], Hbeta, and [OIII]5007
emission lines (ezMOS_avg)
268- 277 A10 --- Structure Kinematical structure in which
the galaxy is located
(Structure) (4)
279- 296 F18.15 mag Bmag ? B-band (CFHT/CFH12k) AUTO
magnitude (Vega system);
automatic aperture from
SExtractor; proxy for total
magnitude (B_AUTO) (1)
298- 318 F21.19 mag e_Bmag ? Error in B-band AUTO magnitude
(eBAUTO) (1)
320- 336 F17.14 mag Vmag ? V-band (CFHT/CFH12k) AUTO
magnitude V_AUTO) (1)
338- 358 F21.19 mag e_Vmag ? Error in V-band AUTO magnitude
(eVAUTO) (1)
360- 377 F18.15 mag Rmag ? R-band (CFHT/CFH12k) AUTO
magnitude (R_AUTO) (1)
379- 398 F20.18 mag e_Rmag ? Error in R-band AUTO magnitude
(eRAUTO) (1)
400- 417 F18.15 mag Imag ? I-band (CFHT/CFH12k) AUTO
magnitude (I_AUTO) (1)
419- 436 F18.16 mag e_Imag ? Error in I-band AUTO magnitude
(eIAUTO) (1)
438- 455 F18.15 mag Jmag ? J-band (Palomar200/WIRC) AUTO
magnitude (J_AUTO) (1)
457- 474 F18.16 mag e_Jmag ? Error in J-band AUTO magnitude
(eJAUTO) (1)
476- 493 F18.15 mag Ksmag ? Ks-band (Palomar200/WIRC) AUTO
magnitude (Ks_AUTO) (1)
495- 512 F18.16 mag e_Ksmag ? Error in Ks-band AUTO magnitude
(eKsAUTO) (1)
514- 531 F18.15 mag F814Wmag ? HST/WFPC2 814nm wide band AUTO
magnitude (F814W_AUTO) (1)
533- 550 F18.16 mag e_F814Wmag ? Error in HST/WFPC2 814nm wide
band AUTO magnitude
(eF814WAUTO) (1)
552- 573 E22.17 mW/m2 FHaSP15 Flux of Halpha emission line
(FHalphaSP15) (1)
575- 596 E22.17 mW/m2 e_FHaSP15 Error in flux of Halpha emission
line (eFHalpha_SP15) (1)
598- 619 E22.17 mW/m2 FNIISP15 ? Flux of [NII]6548 emission line
(FNIISP15) (1)
621- 641 E21.16 mW/m2 e_FNIISP15 ? Error in flux of [NII]6548
emission line (eFNIISP15) (1)
643- 664 E22.17 mW/m2 FHacSP15 Flux of Halpha adjusted and
corrected for absorptions and
extinction
(FHalphacorrectedSP15) (1)
666- 687 E22.17 mW/m2 e_FHacSP15 Error in flux of Halpha adjusted
and corrected for absorptions and
extinction
(eFHalphacorrectedSP15) (1)
689- 710 E22.17 mW/m2 FNIIcSP15 ? Flux of [NII]6548 adjusted and
corrected for absorptions and
extinction
(FNIIcorrectedSP15) (1)
712- 733 E22.17 mW/m2 e_FNIIcSP15 ? Error in flux of [NII]6548
adjusted and corrected for
absorptions and extinction
(eFNIIcorrectedSP15) (1)
735- 744 F10.6 0.1nm EWHaSP15 Equivalent width of Halpha
emission line obtained from
tunable filters
(EWHalphaSP15) (1)
746- 754 F9.6 0.1nm e_EWHaSP15 Error in equivalent width of
Halpha emission line obtained
from tunable filters
(eEWHalpha_SP15) (1)
756- 777 E22.17 10mW/m2/nm ContHaIC Continuum level of Halpha line
obtained from inverse convolution
(ContHalphaInvConv) (3)
779- 800 E22.17 10mW/m2/nm b_ContHaIC Lower value of continuum level of
Halpha line obtained from
inverse convolution
(ContHalphaInvConv_d) (3)
802- 823 E22.17 10mW/m2/nm B_ContHaIC Upper value of continuum level of
Halpha line obtained from
inverse convolution
(ContHalphaInvConv_u) (3)
825- 833 F9.6 0.1nm sigmaHaIC Sigma of the Gaussian fit for
Halpha line obtained from
inverse convolution
(sigmaHalphaInvConv) (3)
835- 843 F9.6 0.1nm b_sigmaHaIC Lower value of sigma of the
Gaussian fit for Halpha line
obtained from inverse convolution
(sigmaHalphaInvConv_d) (3)
845- 853 F9.6 0.1nm B_sigmaHaIC Upper value of sigma of the
Gaussian fit for Halpha line
obtained from inverse convolution
(sigmaHalphaInvConv_u) (3)
855- 876 E22.17 mW/m2 FNII6548IC Flux of [NII]6548 emission line
obtained from inverse convolution
(FNII6548InvConv) (3)
878- 899 E22.17 mW/m2 b_FNII6548IC Lower value of flux of [NII]6548
emission line obtained from
inverse convolution
(FNII6548InvConv_d) (3)
901- 922 E22.17 mW/m2 B_FNII6548IC Upper value of flux of [NII]6548
emission line obtained from
inverse convolution
(FNII6548InvConv_u) (3)
924- 945 E22.17 mW/m2 FHaIC Flux of Halpha emission line
obtained from inverse convolution
(FHalphaInvConv) (3)
947- 957 E11.6 mW/m2 b_FHaIC Lower value of flux of Halpha
obtained from inverse convolution
(FHalphaInvConv_d) (3)
959- 980 E22.17 mW/m2 B_FHaIC Upper value of flux of Halpha
obtained from inverse convolution
(FHalphaInvConv_u) (3)
982-1003 E22.17 mW/m2 FNII6583IC Flux of [NII]6583 emission line
obtained from inverse convolution
(FNII6583InvConv) (3)
1005-1026 E22.17 mW/m2 b_FNII6583IC Lower value of flux of [NII]6583
obtained from inverse convolution
(FNII6583InvConv_d) (3)
1028-1049 E22.17 mW/m2 B_FNII6583IC Upper value of flux of [NII]6583
obtained from inverse convolution
(FNII6583InvConv_u) (3)
1051-1058 E8.6 0.1nm EWNII6548IC Equivalent width of [NII]6548
emission line obtained from
inverse convolution
(EWNII6548InvConv) (3)
1060-1070 E11.6 0.1nm b_EWNII6548IC Lower value of equivalent width of
[NII]6548 emission line obtained
from inverse convolution
(EWNII6548InvConv_d) (3)
1072-1080 F9.6 0.1nm B_EWNII6548IC Upper value of equivalent width of
[NII]6548 emission line
obtained from inverse convolution
(EWNII6548InvConv_u) (3)
1082-1091 F10.6 0.1nm EWHaIC Equivalent width of Halpha
emission line obtained from
inverse convolution
(EWHalphaInvConv) (3)
1093-1100 E8.6 0.1nm b_EWHaIC Lower value of equivalent width of
Halpha emission line obtained
from inverse convolution
(EWHalphaInvConv_d) (3)
1102-1110 F9.5 0.1nm B_EWHaIC Upper value of equivalent width of
Halpha emission line obtained
from inverse convolution
(EWHalphaInvConv_u) (3)
1112-1120 F9.6 0.1nm EWNII6583IC Equivalent width of [NII]6583
emission line obtained from
inverse convolution
(EWNII6583InvConv) (3)
1122-1132 E11.9 0.1nm b_EWNII6583IC Lower value of equivalent width of
[NII]6583 emission line obtained
from inverse convolution
(EWNII6583InvConv_d) (3)
1134-1142 F9.6 0.1nm B_EWNII6583IC Upper value of equivalent width of
[NII]6583 emission line obtained
from inverse convolution
(EWNII6583InvConv_u) (3)
1144-1163 F20.15 0.1nm EWOII ? Equivalent width of [OII]
emission line (EW_OII)
1165-1184 F20.16 0.1nm e_EWOII ? Error in equivalent width of
[OII] emission line (eEWOII)
1186-1205 F20.16 0.1nm EWHb ? Equivalent width of Hbeta
emission line (EW_Hbeta)
1207-1225 F19.16 0.1nm e_EWHb ? Error in equivalent width of
Hbeta emission line (eEWHbeta)
1227-1246 F20.16 0.1nm EWOIII ? Equivalent width of [OIII]5007
emission line (EW_OIII)
1248-1266 F19.16 0.1nm e_EWOIII ? Error in equivalent width of
[OIII]5007 emission line
(eEWOIII)
1268-1286 F19.16 10mW/m2/nm contOII ? Continuum level of [OII]
emission line (cont_OII)
1288-1305 F18.16 10mW/m2/nm e_contOII ? Error in continuum level of
[OII] emission line (econtOII)
1307-1325 F19.16 10mW/m2/nm contHb ? Continuum level of Hbeta
emission line (cont_Hbeta)
1327-1344 F18.16 10mW/m2/nm e_contHb ? Error in continuum level of
Hbeta emission line
(econtHbeta)
1346-1364 F19.16 10mW/m2/nm contOIII ? Continuum level of [OIII]5007
emission line (cont_OIII)
1366-1383 F18.16 10mW/m2/nm e_contOIII ? Error in continuum level of
[OIII]5007 emission line
(econtOIII)
1385-1403 F19.16 10mW/m2/nm coreOII ? Core (amplitude) of [OII]
emission line (core_OII)
1405-1422 F18.16 10mW/m2/nm e_coreOII ? Error in core (amplitude) of
[OII] emission line (ecoreOII)
1424-1442 F19.16 10mW/m2/nm coreHb ? Core (amplitude) of Hbeta
emission line (core_Hbeta)
1444-1461 F18.16 10mW/m2/nm e_coreHb ? Error in core (amplitude) of
Hbeta emission line
(ecoreHbeta)
1463-1482 F20.16 10mW/m2/nm coreOIII ? Core (amplitude) of [OIII]5007
emission line (core_OIII)
1484-1501 F18.16 10mW/m2/nm e_coreOIII ? Error in core (amplitude) of
[OIII]5007 emission line
(ecoreOIII)
1503-1520 F18.16 0.1nm sigmaOII ? sigma of the Gaussian fit for
[OII] emission line (sigma_OII)
1522-1539 F18.16 0.1nm e_sigmaOII ? Error in sigma of the Gaussian
fit for [OII] emission line
(esigmaOII)
1541-1558 F18.16 0.1nm sigmaHb ? sigma of the Gaussian fit for
Hbeta emission line (sigma_Hbeta)
1560-1578 F19.16 0.1nm e_sigmaHb ? Error in sigma of the Gaussian
fit for Hbeta emission line
(esigmaHbeta)
1580-1597 F18.16 0.1nm sigmaOIII ? sigma of the Gaussian fit for
[OIII]5007 emission line
(sigma_OIII)
1599-1616 F18.16 0.1nm e_sigmaOIII ? Error in sigma of the Gaussian
fit for [OIII]5007 emission line
(esigmaOIII)
1618-1635 F18.15 0.1nm FWHMOII ? Full-Width at Half Maximum
(FWHM) of the Gaussian fit for
[OII] emission line (FWHM_OII)
1637-1654 F18.16 0.1nm e_FWHMOII ? Error in FWHM of the Gaussian
fit for [OII] emission line
(eFWHMOII)
1656-1673 F18.15 0.1nm FWHMHb ? Full-Width at Half Maximum
(FWHM) of the Gaussian fit for
Hbeta emission line (FWHM_Hbeta)
1675-1693 F19.16 0.1nm e_FWHMHb ? Error in FWHM of the Gaussian
fit for Hbeta emission line
(eFWHMHbeta)
1695-1712 F18.15 0.1nm FWHMOIII ? Full-Width at Half Maximum
(FWHM) of the Gaussian fit for
[OIII]5007 emission line
(FWHM_OIII)
1714-1731 F18.16 0.1nm e_FWHMOIII ? Error in FWHM of the Gaussian
fit for [OIII]5007 emission line
(eFWHMOIII)
1733-1751 F19.15 --- SNRlineOII ? Signal-to-Noise Ratio (S/N) of
the [OII] emission line
(SNRlineOII)
1753-1772 F20.16 --- SNRlineHb ? Signal-to-Noise Ratio (S/N) of
the Hbeta emission line
(SNRlineHbeta)
1774-1792 F19.16 --- SNRlineOIII ? Signal-to-Noise Ratio (S/N) of
the [OIII]5007 emission line
(SNRlineOIII)
1794-1815 E22.17 mW/m2 FOII ? Flux of [OII] emission line
(F_OII)
1817-1838 E22.17 mW/m2 e_FOII ? Error in flux of [OII] emission
line (eFOII)
1840-1861 E22.17 mW/m2 FHb ? Flux of Hbeta emission line
(F_Hbeta)
1863-1884 E22.17 mW/m2 e_FHb ? Error in flux of Hbeta emission
line (eFHbeta)
1886-1907 E22.17 mW/m2 FHblim ? Upper-limit flux of Hbeta
(if no fitting was performed)
(FHbetalim)
1909-1930 E22.17 mW/m2 FOIII ? Flux of [OIII]5007 emission line
(F_OIII)
1932-1953 E22.17 mW/m2 e_FOIII ? Error in flux of [OIII]5007
emission line (eFOIII)
1955-1976 E22.17 mW/m2 FOIIIlim ? Upper-limit flux of [OIII]5007
(if no fitting was performed)
(FOIIIlim)
1978-1999 E22.17 mW/m2 FOIIadj ? Flux of [OII] emission line
adjusted for aperture effect
(FOIIadj) (5)
2001-2022 E22.17 mW/m2 e_FOIIadj ? Error in flux of [OII] emission
line adjusted for aperture effect
(eFOII_adj) (5)
2024-2045 E22.17 mW/m2 FHbadj ? Flux of Hbeta emission line
adjusted for aperture effect
(FHbetaadj) (5)
2047-2068 E22.17 mW/m2 e_FHbadj ? Error in flux of Hbeta emission
line adjusted for aperture effect
(eFHbeta_adj) (5)
2070-2091 E22.17 mW/m2 FHbadjlim ? Upper-limit flux of Hbeta
adjusted for aperture effect
(if no fitting was performed)
(FHbetalim_adj) (4)
2093-2114 E22.17 mW/m2 FOIIIadj ? Flux of [OIII]5007 emission line
adjusted for aperture effect
(FOIIIadj) (5)
2116-2137 E22.17 mW/m2 e_FOIIIadj ? Error in flux of [OIII]5007
emission line adjusted for
aperture effect
(eFOI )5)II_adj) (5)
2139-2160 E22.17 mW/m2 FOIIIadjlim ? Upper-limit flux of [OIII]5007
adjusted for aperture effect
(if no fitting was performed)
(FOIIIlim_adj) (4)
2162-2183 E22.17 mW/m2 FHaabs ? Flux of Halpha emission line
adjusted and corrected for
absorption (FHalphaabs) (3)
2185-2206 E22.17 mW/m2 e_FHaabs ? Error in flux of Halpha emission
line adjusted and corrected for
absorption (eFHalpha_abs) (3)
2208-2229 E22.17 mW/m2 FHbabs ? Flux of Hbeta emission line
adjusted and corrected for
absorption (FHbetaabs)
2231-2252 E22.17 mW/m2 e_FHbabs ? Error in flux of Hbeta emission
line adjusted and corrected for
absorption (eFHbeta_abs)
2254-2274 E21.16 mW/m2 FHbabslim ? Upper-limit flux of Hbeta
adjusted and corrected for
absorption (if no fitting was
performed) (FHbetalim_abs)
2276-2297 E22.17 mW/m2 FNII6548ec ? Flux of [NII]6548 emission line
adjusted and corrected for
absorptions and extinction
(FNII6548extinc) (3)
2299-2320 E22.17 mW/m2 e_FNII6548ec ? Error in flux of [NII]6548
emission line adjusted and
corrected for absorptions and
extinction
(eFNII6548_extinc) (3)
2322-2343 E22.17 mW/m2 FHaec ? Flux of Halpha emission line
adjusted and corrected for
absorptions and extinction
(FHalphaextinc)
2345-2366 E22.17 mW/m2 e_FHaec ? Error in flux of Halpha emission
line adjusted and corrected for
absorptions and extinction
(eFHalpha_extinc) (3)
2368-2389 E22.17 mW/m2 FNII6583ec Flux of [NII]6583 emission line
adjusted and corrected for
absorptions and extinction
(FNII6583extinc) (3)
2391-2412 E22.17 mW/m2 e_FNII6583ec Error in flux of [NII]6583
emission line adjusted and
corrected for absorptions and
extinction
(eFNII6583_extinc) (3)
2414-2435 E22.17 mW/m2 FOIIec ? Flux of [OII] emission line
adjusted and corrected for
absorptions and extinction
(FOIIextinc)
2437-2458 E22.17 mW/m2 e_FOIIec ? Error in flux of [OII] emission
line adjusted and corrected for
absorptions and extinction
(eFOII_extinc)
2460-2481 E22.17 mW/m2 FHbec ? Flux of Hbeta emission line
adjusted and corrected for
absorptions and extinction
(FHbetaextinc)
2483-2504 E22.17 mW/m2 e_FHbec ? Error in flux of Hbeta emission
line adjusted and corrected for
absorptions and extinction
(eFHbeta_extinc)
2506-2527 E22.17 mW/m2 FHbeclim ? Upper-limit flux of Hbeta
adjusted and corrected for
absorptions and extinction
(if no fitting was performed)
(FHbetalim_extinc)
2529-2550 E22.17 mW/m2 FOIIIec ? Flux of [OIII]5007 emission line
adjusted and corrected for
absorptions and extinction
(FOIIIextinc)
2552-2573 E22.17 mW/m2 e_FOIIIec ? Error in flux of [OIII]5007
emission line adjusted and
corrected for absorptions and
extinction (eFOIII_extinc)
2575-2596 E22.17 mW/m2 FOIIIeclim ? Upper-limit flux of [OIII]5007
adjusted and corrected for
absorptions and extinction
(if no fitting was performed)
(FOIIIlim_extinc)
2598-2615 F18.16 --- FluxadjfacOII ? Flux adjustment factor for
[OII] emission line
(fluxadjfactor_OII) (5)
2617-2634 F18.16 --- FluxadjfacHb ? Flux adjustment factor for Hbeta
emission line
(fluxadjfactor_Hbeta) (5)
2636-2653 F18.16 --- FluxadjfacOIII ? Flux adjustment factor for
[OIII]5007 emission line
(fluxadjfactor_OIII) (5)
2655-2658 F4.2 0.1nm EWabsHaCSP ? Equivalent width of Halpha line
obtained from CSP
(EWabsHalpha_CSP)
2660-2663 F4.2 0.1nm EWabsHbCSP ? Equivalent width of Hbeta line
obtained from CSP
(EWabsHbeta_CSP)
2665-2683 F19.16 --- E(B-V)Balmer ? Balmer decrement- derived color
excess of the stellar continuum
(EBV_Balmer)
2685-2702 F18.16 --- E(B-V)CSP ? Color excess of the stellar
continuum obtained from CSP
(EBV_CSP)
2704-2721 F18.16 --- E(B-V)used ? Color excess of the stellar
continuum used to apply
correction of extinction
(EBV_used)
2723-2728 A6 --- FlagE(B-V) Flag indicating the source of
E(BVused: "Balmer" for Balmer
decrement, "CSP" for CSP
(flag_EBV)
2730-2747 F18.15 [Msun] logM* ? Logarithm of the stellar mass
obtained from CSP
(logStellar_mass)
2749-2768 F20.18 [Msun] e_logM* ? Error in logarithm of the
stellar mass obtained from
CSP (elogStellarmass)
2770-2787 F18.16 --- D4000 ? D4000 break index (D4000)
2789-2806 F18.16 --- e_D4000 ? Error in D4000 break index
(e_D4000)
2808-2814 F7.5 --- MetN2IC ? N2 metallicity (12+log(O/H))
from inverse convolution
(MetN2InvConv) (3)
2816-2822 F7.5 --- b_MetN2IC Lower value of N2 metallicity
(12+log(O/H)) from inverse
convolution
(MetN2InvConv_d) (3)
2824-2830 F7.5 --- B_MetN2IC Upper value of N2 metallicity
(12+log(O/H)) from inverse
convolution
(MetN2InvConv_u) (3)
2832-2849 F18.16 --- MetP05 ? P05 metallicity (12+log(O/H))
(Met_P05)
2851-2872 F22.10 --- e_MetP05 ? Error in P05 metallicity
(12+log(O/H)) (eMetP05)
2874-2890 F17.15 --- MetZ94 ? Z94 metallicity (12+log(O/H))
(Met_Z94)
2892-2909 F18.16 --- e_MetZ94 ? Error in Z94 metallicity
(12+log(O/H)) (eMetZ94)
2911-2927 F17.15 --- MetM91 ? M91 metallicity (12+log(O/H))
(Met_M91)
2929-2946 F18.16 --- e_MetM91 ? Error in M91 metallicity
(12+log(O/H)) (eMetM91)
2948-2964 F17.15 --- MetPP04 ? PP04 metallicity (12+log(O/H))
(Met_PP04)
2966-2983 F18.16 --- e_MetPP04 ? Error in PP04 metallicity
(12+log(O/H)) (eMetPP04)
2985-3001 F17.15 --- MetT04 ? T04 metallicity (12+log(O/H))
(Met_T04)
3003-3020 F18.16 --- e_MetT04 ? Error in T04 metallicity
(12+log(O/H)) (eMetT04)
3022-3040 F19.16 Msun/yr SFRHa ? Halpha star formation rate
(Kennicutt & Evans,
2012ARA&A..50..531K 2012ARA&A..50..531K) (SFR_Ha)
3042-3059 F18.16 Msun/yr e_SFRHa ? Error in Halpha star formation
rate based on Halpha (Kennicutt &
Evans, 2012ARA&A..50..531K 2012ARA&A..50..531K)
(eSFRHa)
3061-3079 F19.16 Msun/yr SFRHb ? Hbeta star formation rate based
(Kennicutt & Evans,
2012ARA&A..50..531K 2012ARA&A..50..531K) (SFR_Hbeta)
3081-3098 F18.16 Msun/yr e_SFRHb ? Error in Hbeta star formation
rate based (Kennicutt & Evans,
2012ARA&A..50..531K 2012ARA&A..50..531K)
(eSFRHbeta)
3100-3118 F19.16 Msun/yr SFROIIZ94 ? [OII] star formation rate
corrected by Z94 (Kewley+2004)
(SFROIIZ94)
3120-3137 F18.16 Msun/yr e_SFROIIZ94 ? Error in [OII] star formation
rate corrected by Z94
(Kewley+2004) (eSFROII_Z94)
3139-3156 F18.16 Msun/yr SFROIIM91 ? [OII] star formation rate
corrected by M91 (Kewley et al.
2004AJ....127.2002K 2004AJ....127.2002K)
(SFROIIM91)
3158-3175 F18.16 Msun/yr e_SFROIIM91 ? Error in [OII] star formation
rate corrected by M91
(Kewley, 2004AJ....127.2002K 2004AJ....127.2002K)
(eSFROII_M91)
3177-3194 F18.14 arcsec Dclusteras Cluster-centric projected distance
in arcsec (Dclusterarcsec) (6)
3196-3213 F18.16 Mpc DclusterMpc Cluster-centric projected distance
in Mpc (DclusterMpc) (6)
3215-3234 F20.16 1/Mpc2 sigma5 Local density estimated to the
5th neighbor (sigma5) (6)
3236-3254 F19.16 1/Mpc2 sigma10 Local density estimated to the
10th neighbor (sigma10) (6)
3256-3258 F3.1 --- isAGNSP15 True/False flag for AGN activity
(isAGN_SP15) (1)
3260-3262 F3.1 --- isBLAGNSP15 True/False flag for broad-line AGN
(isBLAGN_SP15) (1)
3264-3266 F3.1 --- isAGNBPT [0/1]? True/False flag for AGN
activity based on BPT
(Kauffmann+2003); NaN if not
conclusive (isAGN_BPT)
3268-3270 F3.1 --- isAGNWHAN [0/1]? True/False flag for AGN
activity based on EWalphaN2
(Ho+1997); NaN if not conclusive
(isAGN_WHAN)
3272-3274 F3.1 --- isSFGMOS [0/1]True/False flag for
star-forming galaxies based on
BPT and EWalphaN2; NaN if not
conclusive (isSFG_MOS)
3276-3278 F3.1 --- isAGNMOS [0/1]True/False flag for AGN
activity based on BPT and
EWalphaN2; NaN if not conclusive
(isAGN_MOS)
3280-3282 F3.1 --- isCompMOS [0/1]? True/False flag for
composite galaxies based on BPT
and EWalphaN2; NaN if not
conclusive (isComposite_MOS)
3284-3286 F3.1 --- isOutlier [0/1] True/False flag for outlier
galaxies (TF redshift not
confident) (is_Outlier)
3288 I1 --- QualIC [1/6] Quality criterion of
inverse convolution
(Quality_InvConv) (3)
--------------------------------------------------------------------------------
Note (1): Values from Sanchez-Portal et al., 2015, Cat. J/A+A/578/A30
Note (2): 'a' or 'b'; see Fig. 4 in Sanchez-Portal et al . 2015A&A...578A..30S 2015A&A...578A..30S,
'C' and 'O', respectively, in Table 5 of Sanchez-Portal et al.,
2015A&A...578A..30S 2015A&A...578A..30S, Cat. J/A+A/578/A30
Note (3): Following the methodology and data described in Cedres et al.,
2024A&A...686A..60C 2024A&A...686A..60C
Note (4): Based on z_avg or, if unavailable, zHalphaInvConv
(if Quality_InvConv<4) or z_SP15 (if Quality_InvConv≥4).
If 0.366<z<0.3876, it is "B", else if z>0.3876, it is "A";
if z<0.366, it is "Interloper"
Note (5): Fluxes were adjusted due to the use of MOS slits, as described in
Appendix B.1.
Note (6): Information provided by Perez-Martinez et al. (in prep.).
--------------------------------------------------------------------------------
Acknowledgements:
Simon B. De Daniloff, sbonnal(at)iram.es
References:
Beyoro-Amado et al., Paper I 2021MNRAS.501.2430B 2021MNRAS.501.2430B, Cat. J/MNRAS/501/2430
Cedres et al., Paper II 2024A&A...686A..60C 2024A&A...686A..60C
(End) Patricia Vannier [CDS] 19-Aug-2025