VizieR

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VizieR

  
J/MNRAS/482/154
  GHASP. spiral galaxies dark matter distribution (Korsaga+, 2019)
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img(gal)
1.J/MNRAS/482/154/tablea2Parameters of mass models using the BFM and fixed M/L techniques with the pseudo-isothermal (ISO) model (100 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)
  ID (char) Name of the galaxy in the UGC catalogue (UGC NNNNN) (meta.id;meta.main)
  f_ID (char) [*] Flag on ID * : galaxies for which the presence of dark matter is not necessary (meta.code)
  M/LdBFM Msun/LsunM/L of the disc from the best-fitting model (BFM) for pseudo-isothermal (ISO) core model (Note 1)   (phys.composition.massLightRatio)
  E_M/LdBFM Msun/LsunUpper error on M/LDBFM (Note 1)   (stat.error;stat.max)
  e_M/LdBFM Msun/LsunLower error on M/LDBFM (Note 1)   (stat.error)
  M/LbBFM Msun/Lsun(n) M/L of the bulge from the best-fitting model (BFM) for pseudo-isothermal (ISO) core model (Note 1)   (phys.composition.massLightRatio)
  E_M/LbBFM Msun/Lsun(n) Upper error on M/LBBFM (Note 1)   (stat.error;stat.max)
  e_M/LbBFM Msun/Lsun(n) Lower error on M/LBBFM (Note 1)   (stat.error)
  l_r0BFM (char) Lower limit flag on r0BFM (Note 1)   (meta.code.error)
  r0BFM kpc Core radius of the dark matter halo from the best-fitting model (BFM) for pseudo-isothermal (ISO) core model (Note 1)   (phys.size.radius)

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(n) indicates a possible blank or NULL column(i)indexed column
  E_r0BFM kpc (n) Upper error on r0BFM (Note 1)   (stat.error;stat.max)
  e_r0BFM kpc (n) Lower error on r0BFM (Note 1)   (stat.error)
  rho0BFM 10-3Msun/pc3Central density of the dark matter halo from the best-fitting model (BFM) for pseudo-isothermal (ISO) core model (Note 1)   (phys.density)
  E_rho0BFM 10-3Msun/pc3Upper error on rho0BFM (Note 1)   (stat.error;stat.max)
  e_rho0BFM 10-3Msun/pc3Lower error on rho0BFM (Note 1)   (stat.error)
  Chi2BFM  Reduced chi-squared from the best-fitting model (BFM) for pseudo-isothermal (ISO) core model (Note 1)   (stat.fit.chi2)
  M/LfML Msun/LsunM/L derived using the B-V colour (Note 2)   (phys.composition.massLightRatio)
  r0fML kpc Core radius of the dark matter halo from pseudo-isothermal (ISO) core model with fixed M/L (Note 3)   (phys.size.radius)
  E_r0fML kpc Upper error on r0fML (Note 3)   (stat.error;stat.max)
  e_r0fML kpc Lower error on r0fML (Note 3)   (stat.error)
  rho0fML 10-3Msun/pc3Central density of the dark matter halo from pseudo-isothermal (ISO) core model with fixed M/L (Note 3)   (phys.density)
  E_rho0fML 10-3Msun/pc3Upper error on rho0fML (Note 3)   (stat.error;stat.max)
  e_rho0fML 10-3Msun/pc3Lower error on rho0fML (Note 3)   (stat.error)
  Chi2fML  Reduced chi-squared from pseudo-isothermal (ISO) core model with fixed M/L (Note 3)   (stat.fit.chi2)

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