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  Subaru obs. of Vesta in MIR spectral range (Palomba+, 2019)
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1.J/ApJ/882/L22/emissivityVesta spectral emissivity from 2016-01-23, 2016-01-24, 2017-01-12 and 2017-01-13 data (Interactive plot) (Note) (946 rows)
2.J/ApJ/882/L22/laboAbsolute emissivity of eucrite NWA7854 with grain size 25-63um and howardite NWA2698 with grain size 0-25um (Interactive plot) (2810 rows)

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Column  Constraint Explain   (UCD)
  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  (1)Date (char) "Y-M-D" Date of the observation (time.epoch)
   (ALL)lambda um [7.67/13.1] Wavelength (em.wl)
   (ALL)em  (n) [0.81/0.96] Emissivity (phys.emissivity)
  (1)e_em  (n) [0.007/0.08] Uncertainty in em (stat.error)
  (1)Tss (char) Tss parameter (
  (1)GE (char) glob. emiss. parameter (
  (1)GR (char) glob. rough. parameter (
  (1)GF (char) glob. fact. parameter (
  (2)Wavenum cm-1 [624.85/3332.56] Wavenumber (em.wavenumber)
  (2)Grain (char) eucrite NWA7854 or howardite NWA2698 (

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