VizieR

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

VizieR

  
J/ApJ/799/72
  Binary AGNs from the VLA Stripe 82 survey (Fu+, 2015)
ReadMe+ftp
2015ApJ...799...72F
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Post annotation 		img(gal)
1.J/ApJ/799/72/table3*Properties of spectroscopically confirmed pairs (Note) (12 rows)

Simple ConstraintList Of Constraints
 
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)
  RName (char) Radio designation (HHMMSS.ss+DDMMSS.s; J2000) (meta.id;meta.main)
  Q (char) [AB] Grade of the candidate binary (Note 1)   (meta.code.qual)
  z   [0.04/0.4] Spectroscopic redshift (src.redshift)
  Inst (char) Instrument used to obtained z: LRIS or SDSS (instr.setup)
  aSep arcsec [2.5/4.6] Angular separation between the optical counterparts in the pair (pos.angDistance)
  pSep kpc [4.1/12] Projected separation in kiloparsecs (pos.distance)
  DelV km/s [20.9/137] Radial velocity separation ΔV (phys.veloc;arith.diff)
  logP1.4 [W/Hz] [22/25] Logarithmic radio power computed from the integrated source flux density at 1.4GHz (phys.luminosity;em.radio;meta.modelled)
  l_logLHa (char) Limit flag on logLHa (meta.code.error)
  logLHa [10-7W] [39.4/42.4] Log Hα luminosity in erg/s; corrected for reddening and aperture-loss (phys.luminosity;em.line.Halpha)
  EWHa 0.1nm [-3/51] Hα equivalent width in the observed frame in Å (spect.line.eqWidth;em.line.Halpha;obs.field)
  e_EWHa 0.1nm [0.1/1.2] EWHa uncertainty (stat.error)
  [NII]/Ha  (n) [0.5/1.7] [NII]λ6584/Hα line flux ratio (phot.flux;arith.ratio;spect.line)
  e_[NII]/Ha  (n) [0.1/0.4] The 1σ error on [NII]/Ha (stat.error)
  [OIII]/Hb  (n) [0.3/1.3] [OIII]λ5007/Hβ line flux ratio (phot.flux;em.line.OIII;arith.ratio)
  e_[OIII]/Hb  (n) [0.1/0.7] The 1σ error on [OIII]/Hb (stat.error)
  Rcl (char) "Excess" or "Normal" Radio classification (Note 2)   (src.class)
  BPTcl (char) Classification based on the BPT line-ratio diagram in Figure 6 (Note 3)   (src.class)

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