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

  NIBLES. I. The Nancay HI survey (van Driel+, 2016)
Post annotation
1.J/A+A/595/A118/tablea5Basic optical and HI data - galaxies with V<850km/s not used for further analysis (6 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)
  sp  Show the spectrum (meta.ref.url)
  Source  Internal source number (
  Flag (char) Flags regarding the SDSS and NRT data (meta.code.error)
  RAJ2000 "h:m:s" (i) Right ascension (J2000.0) (pos.eq.ra;meta.main)
  DEJ2000 "d:m:s" (i) Declination (J2000.0) (pos.eq.dec;meta.main)
  Name (char) common catalog name, other than the SDSS (
  Vopt km/s Optical heliocentric radial velocity, cz (spect.dopplerVeloc.opt;pos.heliocentric)
  e_Vopt km/s Uncertainty in Vopt (stat.error)
  g-r mag (n) SDSS g-r band color, based on model magnitudes (phot.color;em.opt.B;em.opt.R)
  gMAG mag SDSS absolute g-band model magnitude (phys.magAbs)

ALL cols
(n) indicates a possible blank or NULL column(i)indexed column
  log(M*) [Msun] (n) Logarithm of the MEDIAN total stellar mass estimate (phys.mass)
  log(sSFR) [1/yr] (n) Logarithm of the specific Star Formation Rate, or SFR/M* (phys.SFR)
  rms mJy rms noise level values of the HI spectra (instr.det.noise)
  VHI km/s Heliocentric HI radial velocity (spect.dopplerVeloc;em.line.HI;spect.line)
  e_VHI km/s Uncertainty in VHI (stat.error)
  W50 km/s HI profile velocity width measured at 50% of the peak level (spect.line.width;em.line.HI)
  W20 km/s HI profile velocity width measured at 20% of the peak level (spect.line.width;em.line.HI)
  FHI Integrated measured HI line flux (phot.flux.density;em.line.HI;spect.line)
  e_FHI Uncertainty in FHI (stat.error)
  SNR  Peak signal-to-noise ratio (stat.snr;stat.max)
  S/N  Signal-to-noise ratio determined taking into account the HI line width (spect.line.width;em.line.HI)
  log(MHI) [Msun] Logarithm of the total HI mass (phys.mass)
  log(MHI/M*)  (n) Logarithm of the ratio of the total HI and stellar masses (phys.mass;arith.ratio)

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