VizieR

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

Simple TargetList Of TargetsFast Xmatch with large catalogs or Simbad
Target Name (resolved by Sesame) or Position:
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NB: The epoch used for the query is the original epoch of the table(s)Radius Box size

  
J/MNRAS/509/4457
  Catalogue of outflows in E+A galaxies (Baron+, 2022)
ReadMe+ftp
2022MNRAS.509.4457B
Similar Catalogs
Post annotation 		img(gal)
1.J/MNRAS/509/4457/mdat1fgMetadata properties part 1 of our 144 galaxies sample (144 rows)
2.J/MNRAS/509/4457/mdat2fg(c)*Metadata properties part 2 of our 144 galaxies sample (Note) (144 rows)
3.J/MNRAS/509/4457/ionIonized outflow properties assuming outflows extent of 0.3, 1.0, 3.0 kpc and the case (r = 1.0 kpc, ne = 103 cm–3) (Note) (144 rows)
4.J/MNRAS/509/4457/neutralNeutral outflow properties assuming outflows extent of 0.3, 1.0, 3.0 kpc (144 rows)

Simple ConstraintList Of Constraints
 
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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)
   (ALL)Id  (n) Identifier number (id) (meta.id;meta.main)
  (1+4)f_Id  (n) [0/1] Flag indicates whether a source is detected in FIR or not (is_detected) (Note 1)   (meta.code)
  (1)log(LSF) [10-7W] (n) Logarthim of the star formation luminosity derived from 60 micron by IRAS, in units of erg/sec (logLSFFIR) (Note 2)   (phys.luminosity;em.IR.30-60um)
  (1)e_log(LSF) [10-7W] Logarithm of the uncertainty of L(SF) (logLSFFIR_err) (Note 2)   (stat.error)
  (1)log(LAGN) [10-7W] Logarithm of the AGN bolometric luminosity in units of erg/sec (log_LAGN) (Note 3)   (phys.luminosity;em.opt)
  (1)e_log(LAGN) [10-7W] Logarithm of the uncertainty of L(AGN) (logLAGNerr) (Note 3)   (stat.error)
  (1)logM*16 [Msun] (n) The 16th percentile of the optical stellar mass distribution (logMopt_p16) (Note 4)   (phys.mass)
  (1)logM*50 [Msun] (n) The median 50th percentile of the optical stellar mass distribution (logMopt_p50) (Note 4)   (phys.mass)
  (1)logM*84 [Msun] (n) The 84th percentile of the optical stellar mass distribution (logMopt_p84) (Note 4)   (phys.mass)
  (2)Plate  Spectroscopic SDSS plate of the object (plate) (pos.parallax.spect;instr.plate)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2)MJD  Spectroscopic SDSS MJD of the object (mjd) (time.epoch)
  (2)Fiber  Spectroscopic SDSS fiberID of the object (fiber) (pos.parallax.spect)
  (2)z  Redshift (redshift) (src.redshift)
  (2)logLW4 [10-7W] The logarithm of the luminosity in W4 band in WISE in units of erg/sec (log_LW4) (phys.luminosity;em.IR)
  (2)e_logLW4 [10-7W] Logarithm of the uncertainty of L(W4) (logLW4err) (stat.error)
  (2)E(B-V) mag E(B-V) color excess towards the stars (ebv_stars) (Note 1)   (phot.color.excess)
  (2)sigma* km/s The stellar velocity dispersion (sigma_stars) (Note 1)   (phys.veloc.dispersion)
  (2)WageY Gyr The luminosity-weighted age of stars younger than 1 Gyr (age_young) (Note 1)   (time.age)
  (2)WageO Gyr The luminosity-weighted age of stars older than 1 Gyr (age_old) (Note 1)   (time.age)
  (2)E(B-V)N mag The E(B-V) color excess towards the narrow kinematic component of the ionized gas (ebvlinesnarrow) (Note 2)   (phot.color.excess)
  (2)LHaN 10-7W The luminosity of the narrow Halpha component in units of erg/sec (LHalphanarrow) (phys.luminosity;em.line.Halpha)
  (2)LOIIIN 10-7W The luminosity of the narrow [OIII] component in units of erg/sec (LOIIInarrow) (phys.luminosity)
  (2)sigmalN km/s The velocity dispersion in the narrow component of the ionized lines (sigmalinesnarrow) (phys.veloc.dispersion)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2)log([NII]/Ha)N [-] The log([NII]/Halpha) ratio for the narrow kinematic component (NIIHalpharatio_narrow) (spect.line.intensity;arith.ratio)
  (2)log([OIII]/Hb)N [-] The log([OIII]/Hbeta) ratio for the narrow kinematic component (OIIIHbetaratio_narrow) (spect.line.intensity;arith.ratio)
  (2)E(B-V)B mag The E(B-V) towards the broad kinematic component of the ionized gas (ebvlinesbroad) (Note 2)   (phot.color.excess)
  (2)LHaB 10-7W The luminosity of the broad Halpha component in units of erg/sec (LHalphabroad) (phys.luminosity;em.line.Halpha)
  (2)LOIIIB 10-7W The luminosity of the broad [OIII] component in units of erg/sec (LOIIIbroad) (phys.luminosity)
  (2)sigmalB km/s The velocity dispersion in the broad component of the ionized lines (sigmalinesbroad) (phys.veloc.dispersion)
  (2)VmaxlB km/s The maximal outflow broad lines velocity (vmaxlines_broad) (Note 3)   (phys.veloc)
  (2)log([NII]/Ha)B [-] The log([NII]/Halpha) ratio for the broad kinematic component (NIIHalpharatio_broad) (spect.line.intensity;arith.ratio)
  (2)log([OIII]/Hb)B [-] The log([OIII]/Hbeta) ratio for the broad kinematic component (OIIIHbetaratio_broad) (spect.line.intensity;arith.ratio)
  (2)Sloan (char) Display the online SDSS-DR17 data for the nearest object (meta.ref.url)
  (2)SimbadName (char) (n)Designation understandable by the Simbad data-base (meta.id)
  (2)_RA deg (i) Positions from SDSS DR12 (right ascension part) (pos.eq.ra;meta.main)
  (2)_DE deg (i) Positions from SDSS DR12 (declination part) (pos.eq.dec;meta.main)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (3+4)r0.3 kpc Assumed outflow extent in kpc (r=0.3) (phys.size.radius)
  (3)Voutr0.3 km/s Outflow velocity in km/sec (voutr=0.3) (Note G4)   (phys.veloc)
  (3)logUr0.3 [-] Logarithm of the ionization parameter (logUr=0.3) (phys.ionizParam)
  (3)ner0.3 cm-3 Electron density (ner=0.3) (phys.density;phys.electron)
  (3+4)Mr0.3 Msun Outflowing gas mass according to the Halpha emission line (Mhalphar=0.3) (Note G3)   (phys.mass)
  (3+4)dM/dtr0.3 Msun/yr Mass outflow rate according to the Halpha emission line (Mdothalphar=0.3) (Note G3)   (arith.rate;phys.mass;spect.line)
  (3+4)dE/dtr0.3 10-7W Kinetic power in the wind according to the Halpha emission line (Edothalphar=0.3) (Note G3)   (phys.luminosity;spect.line)
  (3+4)r1.0 kpc Assumed outflow extent in kpc (r=1.0) (phys.size.radius)
  (3)Voutr1.0 km/s Outflow velocity in km/sec (voutr=1.0) (Note G4)   (phys.veloc)
  (3)logUr1.0 [-] Logarithm of the ionization parameter (logUr=1.0) (phys.ionizParam)
  (3)ner1.0 cm-3 Electron density (ner=1.0) (phys.density;phys.electron)
  (3+4)Mr1.0 Msun Outflowing gas mass according to the Halpha emission line (Mhalphar=1.0) (Note G3)   (phys.mass)
  (3+4)dM/dtr1.0 Msun/yr Mass outflow rate according to the Halpha emission line (Mdothalphar=1.0) (Note G3)   (arith.rate;phys.mass;spect.line)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (3+4)dE/dtr1.0 10-7W Kinetic power in the wind according to the Halpha emission line (Edothalphar=1.0) (Note G3)   (phys.luminosity;spect.line)
  (3+4)r3.0 kpc Assumed outflow extent in kpc (r=3.0) (phys.size.radius)
  (3)Voutr3.0 km/s Outflow velocity in km/sec (voutr=3.0) (Note G4)   (phys.veloc)
  (3)logUr3.0 [-] Logarithm of the ionization parameter (logUr=3.0) (phys.ionizParam)
  (3)ner3.0 cm-3 Electron density (ner=3.0) (phys.density;phys.electron)
  (3+4)Mr3.0 Msun Outflowing gas mass according to the Halpha emission line (Mhalphar=3.0) (Note G3)   (phys.mass)
  (3+4)dM/dtr3.0 Msun/yr Mass outflow rate according to the Halpha emission line (Mdothalphar=3.0) (Note G3)   (arith.rate;phys.mass;spect.line)
  (3+4)dE/dtr3.0 10-7W Kinetic power in the wind according to the Halpha emission line (Edothalphar=3.0) (Note G3)   (phys.luminosity;spect.line)
  (3)r1.0-n1000 kpc Assumed outflow extent in kpc (r=1.0) (phys.size.radius)
  (3)Voutr1.0-n1000 km/s Outflow velocity in km/sec (vout_r=1.0,n=1000) (Note G4)   (phys.veloc)
  (3)logUr1.0-n1000 [-] Logarithm of the ionization parameter (logUr=1.0,n=1000) (phys.ionizParam)
  (3)ne1000 cm-3 Electron density (ne=1000) (phys.density;phys.electron)
  (3)Mr1.0-n1000 Msun Outflowing gas mass according to the Halpha emission line (Mhalphar=1.0,n=1000) (Note G3)   (phys.mass)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (3)dM/dtr1.0-n1000 Msun/yr Mass outflow rate according to the Halpha emission line (Mdothalphar=1.0,n=1000) (Note G3)   (arith.rate;phys.mass;spect.line)
  (3)dE/dtr1.0-n1000 10-7W Kinetic power in the wind according to the Halpha emission line (Edothalphar=1.0,n=1000) (Note G3)   (phys.luminosity;spect.line)
  (4)Vmaxr0.3 km/s (n) Maximum outflow velocity (Vmaxr=0.3) (Note G1)   (phys.veloc;stat.max)
  (4)NHIr0.3 cm-2 (n) Hydrogen column density extracted from the NaID fitting (NHIr=0.3) (Note G2)   (phys.columnDensity)
  (4)Cfr0.3  (n) Local covering fraction related to wind clumpiness extracted from the spectrum NaID fitting (Cfr=0.3) (phys.size;arith.ratio)
  (4)Vmaxr1.0 km/s (n) Maximum outflow velocity (Vmaxr=1.0) (Note G1)   (phys.veloc;stat.max)
  (4)NHIr1.0 cm-2 (n) Hydrogen column density extracted from the NaID fitting (NHIr=1.0) (Note G2)   (phys.columnDensity)
  (4)Cfr1.0  (n) Local covering fraction related to wind clumpiness extracted from the spectrum NaID fitting (Cfr=1.0) (phys.size;arith.ratio)
  (4)Vmaxr3.0 km/s (n) Maximum outflow velocity (Vmaxr=3.0) (Note G1)   (phys.veloc;stat.max)
  (4)NHIr3.0 cm-2 (n) Hydrogen column density extracted from the NaID fitting (NHIr=3.0) (Note G2)   (phys.columnDensity)
  (4)Cfr3.0  (n) Local covering fraction related to wind clumpiness extracted from the spectrum NaID fitting (Cfr=3.0) (phys.size;arith.ratio)

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