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J/MNRAS/417/2239
 SPIRE (f250um>17.4mJy) GOODS-N galaxies (Symeonidis+, 2011)
Post annotation
img(gal)
1.J/MNRAS/417/2239/table2SPIRE sample of 84 SPIRE-detected, submm-bright (f250um>17.4mJy) galaxies in the GOODS-N field, observed as part of the Herschel/HerMES survey (84 rows)

 
Query by Constraints constraints help applied on Columns (Output Order: + - )
ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  Seq   [1/84] Sequential number, [SGS2011] NN in Simbad (meta.record)
  RAJ2000 deg IRAS 3.6um right ascension in decimal degrees (J2000) (pos.eq.ra;meta.main)
  DEJ2000 deg IRAS 3.6um declination in decimal degrees (J2000) (pos.eq.dec;meta.main)
  z  (n) Spectroscopic redshift (available only for 67 sources) (src.redshift)
  logLIR [Lsun] (n) Total IR luminosity (8-1000um) (phys.luminosity;em.IR)
  HDF-N  (n) Cross-matched ID from the IC catalogue of Hubble Deep Field-North (HDF-N) Chandra data (meta.id.cross)
  l_FSX (char) Limit flag on FSX (3σ limit) (meta.code.error)
  FSX mW/m2 Flux in the soft band (0.5-2keV) (phot.flux;em.X-ray.soft)
  l_FHX (char) Limit flag on FHX (3σ limit) (meta.code.error)
  FHX mW/m2 Flux in the hard band (2-7keV) (phot.flux;em.X-ray.hard)

ALL cols
    
(n) indicates a possible blank or NULL column  
  logLSX [10-7W] (n) Luminosity in soft band (0.5-2keV) (phys.luminosity)
  logLHX [10-7W] (n) Luminosity in hard band (2-7keV) (phys.luminosity)
  HR  (n) Hardness ratio, (H-S)/(H+S) (phot.flux;arith.ratio)
  E_HR  (n) Error on HR (upper value) (stat.error;stat.max)
  e_HR  (n) Error on HR (lower value) (stat.error)
  FHX/FR  (n) fHX/fR ratio used to identify AGN (Note 1)   (phot.flux;arith.ratio)
  E_FHX/FR  (n) Error on FHX/FR (upper value) (stat.error;stat.max)
  e_FHX/FR  (n) Error on FHX/FR (lower value) (stat.error)
  Class (char) Spectral class (Note 2)   (src.class)
  XClass (char) X-ray class (Note 3)   (src.class)

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