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  Lyα emitters at z=6.5 in Subaru Deep Field (Kashikawa+, 2006)
Post annotation
1.J/ApJ/648/7/table2Spectroscopic Properties of z=6.5 LAEs (8 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)
  [TAN2005]  Sequential number (meta.record)
  SDF (char) SDF designation (JHHMMSS.s+DDMMSS) (
  z  Redshift (Note 1)   (src.redshift)
  F(Lya) 10-21W/m2Observed line flux in Lyα (Note 2)   (phot.flux;em.UV)
  L(Lya) 10+35W Estimated Lyα luminosity (Note 3)   (phys.luminosity;em.UV)
  SFR(Lya) solMass/yrLyα Stellar Formation Rate (3) (Note 4)   (arith.rate;phys.SFR)
  FWHM 0.1nm FWHM in Angstroem (Note 5)   (spect.line.width)
  FWHM2 km/s FWHM in km/s (Note 5)   (spect.line.width)
  Sw 0.1nm (n) Weighted skewness (quantifies the asymmetry of the emission lines) (meta.note)
  e_Sw 0.1nm rms uncertainty on Sw (stat.error)
  Obs (char) [FD] Observed with FOCAS (F) or DEIMOS (D) (;instr)
  _RA deg (i) Right ascension (derived from SDF) for Eq=J2000 (pos.eq.ra;meta.main)
  _DE deg (i) Declination (derived from SDF) for Eq=J2000 (pos.eq.dec;meta.main)

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