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  LVHIS. far-infrared radio correlation (Shao+, 2018)
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1.J/MNRAS/479/3509/table4Derived galaxy properties of gold sample (17 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)
  LVHIS   [001/082] LVHIS ID (;meta.main)
  Name (char) Optical counterpart (
  logMstar [Msun] Stellar mass (phys.mass)
  e_logMstar [Msun] Uncertainty of stellar mass (stat.error)
  logSFR [Msun/yr]Star formation rate (phys.SFR)
  e_logSFR [Msun/yr]Uncertainty of tar formation rate (stat.error;phys.SFR)
  logMHI [Msun] HI mass (phys.mass)
  e_logMHI [Msun] Uncertainty of HI mass (stat.error)
  cons  Stellar light concentration (phys.size;arith.ratio)
  e_cons  Uncertainty of stellar light concentration (stat.error)
  D25 kpc 25mag/arcsec^2 diameter in B band (phys.angSize)
  e_D25 kpc Uncertainty of 25mag/arcsec^2 diameter in B band (stat.error)
  RUV kpc FUV 50 percent light radius (phys.size.radius)
  e_RUV kpc Uncertainty of FUV 50 percent light radius (stat.error)
  logmustar [Msun/kpc2]Stellar mass surface density (phys.density)
  e_logmustar [Msun/kpc2]Uncertainty of stellar mass surface density (stat.error)
  logmuSFR [Msun/yr/kpc2]Star formation rate surface density (phys.SFR)
  e_logmuSFR [Msun/yr/kpc2]Uncertainty of star formation rate surface density (stat.error)

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