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J/A+A/527/A139
  X-ray bursting neutron star atmosphere models (Suleimanov+, 2011)
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2011A&A...527A.139S
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1.J/A+A/527/A139/setSet parameters[spectrum] (18 rows)
2.J/A+A/527/A139/tablea1Color and dilution factors (360 rows)
3.J/A+A/527/A139/tablea2*Atmosphere model spectra (Note) (4968 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)
   (ALL)Set  (i) [1/18] Set number linkRole{colors, spectra and dilution factors } (meta.id;meta.main)
  (1)X  X (H) abundance (0, 0.7374, 1) (phys.abund.X)
  (1)Y  Y (He) abundance (0, 0.2492, 0.2586, 0.2613, 0.2625, 1) (phys.abund.Y)
  (1)Z  Z abundance (0, 1.34E-2, 4.02E-3, 1.34E-3, 1.34E-4) (src.redshift)
  (1)logg [cm/s2] Surface gravity (14.0, 14.3, 14.6) (phys.gravity)
  (1)Tedd keV Eddington temperature (9 values) (phys.temperature.effective)
  (1)R km Neutron star radius (8.16, 10.88, 14.80) (phys.size.radius)
  (1)z  Redshift (0.18, 0.27, 0.42) (src.redshift)
  (1)Sp (char)
spectrum
Plot of the spectrum corresponding to this set (meta.ref.url)
  (2)l  Relative luminosity L/Ledd (Note 1)   (phys.luminosity;arith.ratio)

ALL cols		    
 (i)indexed column
  (2)Teff keV Effective temperature (phys.temperature.effective)
  (2)fc1  Color correction factor fc,1 (Note 2)   (arith.factor;phot.flux)
  (2)fc2  Color correction factor fc,2 (Note 2)   (arith.factor;phot.flux)
  (2)fc3  Color correction factor fc,3 (Note 2)   (arith.factor;phot.flux)
  (2)fc4  Color correction factor fc,4 (Note 2)   (arith.factor;phot.flux)
  (2)fc5  Color correction factor fc,5 (Note 2)   (arith.factor;phot.flux)
  (2)w*fc1+4  Product of dilution factor and (fc1)4 (arith.factor;pos.distance)
  (2)w*fc2+4  Product of dilution factor and (fc2)4 (arith.factor;pos.distance)
  (2)w*fc3+4  Product of dilution factor and (fc3)4 (arith.factor;pos.distance)
  (3)E keV Photon energy (em.energy)
  (3)F(001) mW/m2/keVFlux FE for l=0.001 (Note 1)   (phot.flux;em.X-ray)
  (3)F(003) mW/m2/keVFlux FE for l=0.003 (Note 1)   (phot.flux;em.X-ray)
  (3)F(010) mW/m2/keVFlux FE for l=0.01 (Note 1)   (phot.flux;em.X-ray)

ALL cols		    
 (i)indexed column
  (3)F(030) mW/m2/keVFlux FE for l=0.03 (Note 1)   (phot.flux;em.X-ray)
  (3)F(050) mW/m2/keVFlux FE for l=0.05 (Note 1)   (phot.flux;em.X-ray)
  (3)F(070) mW/m2/keVFlux FE for l=0.07 (Note 1)   (phot.flux;em.X-ray)
  (3)F(100) mW/m2/keVFlux FE for l=0.1 (Note 1)   (phot.flux;em.X-ray)
  (3)F(150) mW/m2/keVFlux FE for l=0.15 (Note 1)   (phot.flux;em.X-ray)
  (3)F(200) mW/m2/keVFlux FE for l=0.2 (Note 1)   (phot.flux;em.X-ray)
  (3)F(300) mW/m2/keVFlux FE for l=0.3 (Note 1)   (phot.flux;em.X-ray)
  (3)F(400) mW/m2/keVFlux FE for l=0.4 (Note 1)   (phot.flux;em.X-ray)
  (3)F(500) mW/m2/keVFlux FE for l=0.5 (Note 1)   (phot.flux;em.X-ray)
  (3)F(600) mW/m2/keVFlux FE for l=0.6 (Note 1)   (phot.flux;em.X-ray)
  (3)F(700) mW/m2/keVFlux FE for l=0.7 (Note 1)   (phot.flux;em.X-ray)
  (3)F(750) mW/m2/keVFlux FE for l=0.75 (Note 1)   (phot.flux;em.X-ray)
  (3)F(800) mW/m2/keVFlux FE for l=0.8 (Note 1)   (phot.flux;em.X-ray)
  (3)F(850) mW/m2/keVFlux FE for l=0.85 (Note 1)   (phot.flux;em.X-ray)
  (3)F(900) mW/m2/keVFlux FE for l=0.9 (Note 1)   (phot.flux;em.X-ray)
  (3)F(950) mW/m2/keVFlux FE for l=0.95 (Note 1)   (phot.flux;em.X-ray)
  (3)F(980) mW/m2/keVFlux FE for l=0.98 (Note 1)   (phot.flux;em.X-ray)

ALL cols		    
 (i)indexed column
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