VizieR

CfA VizieR . ADAC VizieR . Cambridge (UK) VizieR . IUCAA VizieR . INASAN VizieR .

VizieR

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NB: The epoch used for the query is the original epoch of the table(s)Radius Box size

  
J/A+A/712/A19
  Chemical composition in low-mass galaxies (Izotov+, 2026)
ReadMe+ftp
2026A&A...712A..19I
Similar Catalogs
Post annotation 		img(gal)
1.J/A+A/712/A19/table1(c)General characteristics of CSFGs galaxies derived from SDSS spectra and GALEX photometry (11 rows)
2.J/A+A/712/A19/tableb1aEmission-line fluxes in 11 galaxies (113 rows)
3.J/A+A/712/A19/tableb1bExtinction coefficients, rest-frame equivalent widths and the observed fluxes of the Hbeta emission line in 11 galaxies (11 rows)
4.J/A+A/712/A19/tableb2Chemical abundances in 11 galaxies (11 rows)

Simple ConstraintList Of Constraints
 
Query by Constraints constraints help applied on Columns (Output Order: + - )
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Column  Constraint Explain   (UCD)
  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  (1+3+4)Name (char) Galaxy CSFGs name (Name) (meta.id;meta.main)
  (1)SDSS (char) Display the SDSS dr16 of Ahumada et al. 2020ApJS..249....3A, Cat. V/154 (meta.ref.url)
  (1)GALEX (char) Display the Revised catalog of GALEX UV sources of Bianchi et al. 2017ApJS..230...24B, Cat. II/335 (meta.ref.url)
  (1)RAJ2000 "h:m:s" (i) Right ascension (J2000) (RA) (pos.eq.ra;meta.main)
  (1)DEJ2000 "d:m:s" (i) Declination (J2000) (Dec) (pos.eq.dec;meta.main)
  (1)z  Redshift (Redshift) (src.redshift)
  (1)gmag mag SDSS g-band magnitude (g) (phot.mag;em.opt.B)
  (1+4)A(O) [-] Oxygen abundance derived by the direct Te-method from the Xshooter spectrum (12+log(O/H)) (phys.abund)
  (1)EWHb 0.1nm Rest-frame equivalent width of the H{beta} emission line in the Xshooter spectrum (EW(H{beta}) (spect.line.eqWidth)
  (1)O32  The oxygen line ratio O32 as [OIII]{lambda}5007/[OII]{lambda}3727 (O32) (meta.note)

ALL cols		    
 (i)indexed column
  (1)logM* [Msun] The stellar mass (logM*) (phys.mass)
  (1)logXi [10+7Hz/J]The logarithm of the production efficiency of ionizing photons (log{Xi}ion) (phys.ionizParam.rad)
  (1)SimbadName (char) (n)Designation understandable by the Simbad data-base (meta.id)
  (2)Line (char) Name of the emission line (Line) (meta.id;spect.line)
  (2)Lambda nm Rest-frame wavelength of the emission line (Lambda) (em.wl;spect.line)
  (2)F01  Flux of the emission line relative to Hbeta emission line in the galaxy J0007+0226 (F01) (phot.flux;spect.line;arith.ratio)
  (2)e_F01  Flux error of the emission line relative to Hbeta emission line in the galaxy J0007+0226 (EF01) (stat.error)
  (2)F02  Flux of the emission line relative to Hbeta emission line in the galaxy J0009+0234 (F02) (phot.flux;spect.line;arith.ratio)
  (2)e_F02  Flux error of the emission line relative to Hbeta emission line in the galaxy J0009+0234 (EF02) (stat.error)
  (2)F03  Flux of the emission line relative to Hbeta emission line in the galaxy J0159+0751 (F03) (phot.flux;arith.ratio;spect.line)
  (2)e_F03  Flux error of the emission line relative to Hbeta emission line in the galaxy J0159+0751 (EF03) (stat.error)
  (2)F04  Flux of the emission line relative to Hbeta emission line in the galaxy J0240-0828 (F04) (phot.flux;spect.line;arith.ratio)
  (2)e_F04  Flux error of the emission line relative to Hbeta emission line in the galaxy J0240-0828 (EF04) (stat.error)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2)F05  Flux of the emission line relative to Hbeta emission line in the galaxy J0825+1846 (F05) (phot.flux;spect.line;arith.ratio)
  (2)e_F05  Flux error of the emission line relative to Hbeta emission line in the galaxy J0825+1846 (EF05) (stat.error)
  (2)F06  Flux of the emission line relative to Hbeta emission line in the galaxy J1255-0213 (F06) (phot.flux;spect.line;arith.ratio)
  (2)e_F06  Flux error of the emission line relative to Hbeta emission line in the galaxy J1255-0213 (EF06) (stat.error)
  (2)F07  Flux of the emission line relative to Hbeta emission line in the galaxy J1310+0852 (F07) (phot.flux;spect.line;arith.ratio)
  (2)e_F07  Flux error of the emission line relative to Hbeta emission line in the galaxy J1310+0852 (EF07) (stat.error)
  (2)F08  Flux of the emission line relative to Hbeta emission line in the galaxy J1323-0132 (F08) (phot.flux;arith.ratio;spect.line)
  (2)e_F08  Flux error of the emission line relative to Hbeta emission line in the galaxy J1323-0132 (EF08) (stat.error)
  (2)F09  Flux of the emission line relative to Hbeta emission line in the galaxy J1325+0744 (F09) (phot.flux;arith.ratio;spect.line)
  (2)e_F09  Flux error of the emission line relative to Hbeta emission line in the galaxy J1325+0744 (EF09) (stat.error)
  (2)F10  Flux of the emission line relative to Hbeta emission line in the galaxy J1411+0550 (F10) (phot.flux;spect.line;arith.ratio)
  (2)e_F10  Flux error of the emission line relative to Hbeta emission line in the galaxy J1411+0550 (EF10) (stat.error)
  (2)F11  Flux of the emission line relative to Hbeta emission line in the galaxy J1526+2113 (F11) (phot.flux;spect.line;arith.ratio)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2)e_F11  Flux error of the emission line relative to Hbeta emission line in the galaxy J1526+2113 (EF11) (stat.error)
  (3)CHb  Extinction coefficient derived from the decrement of hydrogen Balmer emission lines (CHB) (phys.absorption)
  (3)e_CHb  Error of extinction coefficient derived from the decrement of hydrogen Balmer emission lines (ECHB) (stat.error)
  (3)EWHb nm Rest-frame equivalent width of the Hbeta emission line (EWHB) (spect.line.eqWidth;em.line.Hbeta)
  (3)e_EWHb nm Error of the rest-frame equivalent width of the Hbeta emission line (EEWHB) (stat.error)
  (3)FHb W/m2 Observed flux of the Hbeta emission line (FHB) (phot.flux;em.line.Hbeta)
  (3)e_FHb W/m2 Error of observed flux of the Hbeta emission line (EFHB) (stat.error)
  (4)TOIII K Electron temperature for OIII ion (TOIII) (phys.temperature.electron;phys.electron)
  (4)e_TOIII K Error of the electron temperature for OIII ion (ETOIII) (stat.error)
  (4)TOII K Electron temperature for OII ion (TOII) (phys.temperature.electron;phys.electron)
  (4)e_TOII K Error of the electron temperature for OII ion (ETOII) (stat.error)
  (4)TSIII K Electron temperature for SIII ion (TSIII) (phys.temperature.electron;phys.electron)
  (4)e_TSIII K Error of the electron temperature for SIII ion (ETSIII) (stat.error)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (4)nSII cm-3 Electron number density derived from the [SII] 671.7/673.1 emission-line ratio (NSII) (phys.density)
  (4)e_nSII cm-3 Error of the electron number density derived from the [SII] 671.7/673.1 emission-line ratio (ENSII) (stat.error)
  (4)nOII cm-3 Electron number density derived from the [OII] 327.6/327.9 emission-line ratio (NOII) (phys.density)
  (4)e_nOII cm-3 Error of the electron number density derived from the [OII] 327.6/327.9 emission-line ratio (ENOII) (stat.error)
  (4)THE5 K Electron temperature for HeII ion derived from five HeI emission lines (THE5) (phys.temperature.electron;phys.electron)
  (4)neHE5 cm-3 Electron number density for HeII ion derived from five HeI emission lines (NEHE5) (phys.density)
  (4)Tau5  Optical depth in He I 3889 emission line derived from five HeI emission lines (TAU5) (phys.absorption.opticalDepth)
  (4)Y5  Weighted mean He mass fraction derived from derived from five HeI emission lines (Y5) (phys.mass;arith.ratio)
  (4)THE6 K Electron temperature for HeII ion derived from six HeI emission lines (THE6) (phys.temperature.electron;phys.electron)
  (4)neHE6 cm-3 Electron number density for HeII ion derived from six HeI emission lines (NEHE6) (phys.density)
  (4)Tau6  Optical depth in in He I 3889 emission line derived from six HeI emission lines (TAU6) (phys.absorption.opticalDepth)
  (4)Y6  Weighted mean He mass fraction derived from derived from six HeI emission lines (Y6) (phys.mass;arith.ratio)
  (4)O+/H+  The O+/H+ abundance ratio (OP) (phys.abund)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (4)e_O+/H+  Error of O+/H+ abundance ratio (EOP) (stat.error;phys.abund)
  (4)O2+/H+  The O2+/H+ abundance ratio (O2P) (phys.abund)
  (4)e_O2+/H+  Error of O2+/H+ abundance ratio (EO2P) (stat.error;phys.abund)
  (4)O3+/H+  The O3+/H+ abundance ratio (O3P) (phys.abund)
  (4)e_O3+/H+  Error of O3+/H+ abundance ratio (EO3P) (stat.error;phys.abund)
  (4)e_A(O) [-] Error of total oxygen abundance 12+log(O/H) (EO) (stat.error)
  (4)N+/H+  The N+/H+ abundance ratio (NP) (phys.abund)
  (4)e_N+/H+  Error of N+/H+ abundance ratio (ENP) (stat.error;phys.abund)
  (4)ICF(N)  Ionisation correction factor ICF(N) of nitrogen (ICFN) (arith.factor)
  (4)log(N/O) [-] The logarithm of N/O abundance ratio (NO) (phys.abund)
  (4)e_log(N/O) [-] Error of log(N/O) abundance ratio (ENO) (stat.error)
  (4)Ne2+/H+  The Ne2+/H+ abundance ratio (NE2P) (phys.abund)
  (4)e_Ne2+/H+  Error of Ne2+/H+ abundance ratio (ENE2P) (stat.error;phys.abund)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (4)ICF(NE)  Ionisation correction factor ICF(Ne) of neon (ICFNE) (arith.factor)
  (4)log(NE/O) [-] The logaritm of Ne/O abundance ratio (NEO) (phys.abund)
  (4)e_log(NE/O) [-] Error of log of Ne/O abundance ratio (ENEO) (stat.error)
  (4)S+/H+  The S+/H+ abundance ratio (SP) (phys.abund)
  (4)e_S+/H+  Error of S+/H+ abundance ratio (ESP) (stat.error;phys.abund)
  (4)S2+/H+6312  The S2+/H+ abundance ratio derived from [SIII]631.2 emission line (S2P6312) (phys.abund)
  (4)e_S2+/H+6312  Error of S2+/H+ abundance ratio derived from [SIII]631.2 emission line (ES2P6312) (stat.error)
  (4)ICF(S)  Ionisation correction factor ICF(S) of sulfur (ICFS) (arith.factor)
  (4)log(S/O6312) [-] The logarithm of S/O abundance ratio using [SIII]631.2 emission line (SO6312) (phys.abund)
  (4)e_log(S/O6312) [-] Error of log of S/O abundance ratio using [SIII]631.2 emission line (ESO6312) (stat.error)
  (4)S2+/H+9069  The S2+/H+ abundance ratio derived from [SIII]906.9 emission line (S2P9069) (phys.abund)
  (4)e_S2+/H+9069  Error of S2+/H+ abundance ratio using [SIII]906.9 emission line (ES2P9069) (stat.error)
  (4)log(S/O9069) [-] The logarithm of S/O abundance ratio using [SIII]906.9 emission line (SO9069) (phys.abund)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (4)e_log(S/O9069) [-] Error of log of S/O abundance ratio using [SIII]906.9 emission line (ESO9069) (stat.error)
  (4)S2+/H+9531  The S2+/H+ abundance ratio derived from [SIII]953.1 emission line (S2P9531) (phys.abund)
  (4)e_S2+/H+9531  Error of S2+/H+ abundance ratio using [SIII]953.1 emission line (ES2P9531) (stat.error)
  (4)log(S/O9531) [-] The logarithm of S/O abundance ratio using [SIII]953.1 emission line (SO9531) (phys.abund)
  (4)e_log(S/O9531) [-] Error of log(S/O9531) abundance ratio using [SIII]953.1 emission line (ESO9531) (stat.error)
  (4)Cl2+/H+  The Cl2+/H+ abundance ratio (CL2P) (phys.abund)
  (4)e_Cl2+/H+  Error of Cl2+/H+ abundance ratio (ECL2P) (stat.error;phys.abund)
  (4)ICF(Cl)  Ionisation correction factor ICF(Cl) of chlorine (ICFCL) (arith.factor)
  (4)log(Cl/O) [-] The logarithm of Cl/O abundance ratio (CLO) (phys.abund)
  (4)e_log(Cl/O) [-] Error of log(Cl/O) abundance ratio (ECLO) (stat.error)
  (4)Ar2+/H+  The Ar2+/H+ abundance ratio (AR2P) (phys.abund)
  (4)e_Ar2+/H+  Error of Ar2+/H+ abundance ratio (EAR2P) (stat.error;phys.abund)
  (4)Ar3+/H+  The Ar3+/H+ abundance ratio (AR3P) (phys.abund)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (4)e_Ar3+/H+  Error of Ar3+/H+ abundance ratio (EAR3P) (stat.error;phys.abund)
  (4)ICF(Ar)  Ionisation correction factor ICF(Ar) of argon (ICFAR) (arith.factor)
  (4)log(Ar/O) [-] The logarithm of Ar/O abundance ratio (ARO) (phys.abund)
  (4)e_log(Ar/O) [-] Error of log(Ar/O) abundance ratio (EARO) (stat.error)
  (4)Fe2+/H+4658  The Fe2+/H+ abundance ratio derived from [FeIII]465.8 emission line (FE2P466) (phys.abund)
  (4)e_Fe2+/H+4658  Error of Fe2+/H+ abundance ratio derived from [FeIII]465.8 emission line (EFE2P466) (stat.error)
  (4)ICF(Fe4658)  Ionisation correction factor ICF(Fe) using [FeIII]465.8 emission line (ICFFE466) (arith.factor)
  (4)log(Fe/O)4658 [-] The logarithm of Fe/O abundance ratio using [FeIII]465.8 emission line (FEO466) (phys.abund)
  (4)e_log(Fe/O)4658 [-] Error of log of Fe/O abundance ratio using [FeIII]465.8 emission line (EFEO466) (stat.error)
  (4)Fe2+/H+  The Fe2+/H+ abundance ratio derived from [FeIII]498.8 emission line (FE2P499) (phys.abund)
  (4)e_Fe2+/H+  Error of Fe2+/H+ abundance ratio derived from [FeIII]498.8 emission line (EFE2P499) (stat.error;phys.abund)
  (4)ICF(Fe4998)  Ionisation correction factor ICF(Fe) of iron (ICFFE499) (arith.factor)
  (4)log(Fe/O)4998 [-] The logarithm of Fe/O abundance ratio using [FeIII]499.8 emission line (FEO499) (phys.abund)
  (4)e_log(Fe/O)4998 [-] Error of log(Fe/O) abundance ratio using [FeIII]499.8 emission line (EFEO499) (stat.error)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
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