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/ApJ/680/939
  Optical spectra of 24um galaxies in COSMOS. I. (Caputi+, 2008)
Post annotation
img(gal)
1.J/ApJ/680/939/table2(c)*The H{beta}4861 and [OIII]5007 line fluxes for the galaxies in our sample for which both line EWs are greater than 5Å (Note) (55 rows) (released 2018-01-02)
[METAtab] [METAcola]
2.J/ApJ/680/939/table3(c)*The H{alpha}6563 and [NII]6584 line fluxes for the galaxies in our sample for which both line EWs are greater than 5Å (Note) (94 rows) (released 2018-01-02)
[METAtab] [METAcola]
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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)
   (ALL)zCOSMOS  zCOSMOS number (meta.id;meta.main)
   (ALL)f_zCOSMOS (char) [*] Flag on zCOSMOS (Note G1)   (meta.code)
   (ALL)zsp  Spectroscopic redshift (src.redshift)
  (1)Hbeta aW/m2 H{beta}4861 flux (Note 1)   (phot.flux)
  (1)e_Hbeta aW/m2 Hbeta uncertainty (stat.error)
  (1)OIII aW/m2 Flux for [OIII]5007 (phot.flux)
  (1)e_OIII aW/m2 OIII uncertainty (stat.error)
   (ALL)l_Lum (char) Limit flag on Lum (meta.code.error)
   (ALL)Lum (char) [-] Logarithm of rest-frame 24um luminosity: log10{nu}L{nu}24um (phys.luminosity;em.IR.15-30um)
   (ALL)Simbad (char) ask the Simbad data-base about this object

ALL cols
    
 (i)indexed column
   (ALL)NED (char) ask the NED data-base about this object
   (ALL)_RA deg (i) Positions from Simbad (right ascension part) (pos.eq.ra;meta.main)
   (ALL)_DE deg (i) Positions from Simbad (declination part) (pos.eq.dec;meta.main)
  (2)Halpha aW/m2 H{alpha}6563 flux (Note 1)   (phot.flux)
  (2)e_Halpha aW/m2 Halpha uncertainty (stat.error)
  (2)NII aW/m2 Flux for [NII]6584 (phot.flux)
  (2)e_NII aW/m2 NII uncertainty (stat.error)
  (2)f_NII (char) [l] Flag not explained in the paper (meta.code)

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-source=J/ApJ/680/939
-ref=VIZ68edf44a2a3a1b
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