VizieR

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VizieR

  
J/MNRAS/522/6326
  MaNGA galaxies DynPop I JAM dynamical properties (Zhu+, 2023)
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1.J/MNRAS/522/6326/table4*Dynamical properties as velocities, inclination angle, M/L,masses and density slopes for JAMcyl+NFW parametrized model (Note) (10296 rows)

 
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ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  ID  Identifier raw number (meta.id;meta.main)
  i deg (n) Best-fitting inclination angle, being 90 for edge-on as modelled in section 3.2 (inc_deg) (src.orbital.inclination;pos.posAng)
  Betaz  (n) Best-fitting radial velocity anisotropy {Beta}zin cylindrical coordinates (beta_z) (phys.veloc;arith.diff)
  logM/Ls [Msun/Lsun](n) Best-fitting stellar mass-to-light ratio in M{sun}/L{sun} units (logMLstellar) (phys.composition.massLightRatio)
  logrhos [Msun/kpc3](n) The characteristic density of NFW profile (logrhos) (phys.density)
  rs kpc (n) The break radius as characteristic radius of NFW profile (rs) (phys.size.radius)
  Kappa  (n) The ratio between modelled and observed line-of-sight velocity field (kappa) (phys.veloc;arith.diff)
  log(Mt<Re) [Msun] (n) Enclosed total stellar matter+DM+BH mass within a sphere of circularized effective radius Re which satisfying that the area of half-light ellipse A={pi}*Re2 (logMtRe) (phys.mass)
  log(Ms<Re) [Msun] (n) Enclosed stellar matter mass within a sphere of circularized effective radius Re which satisfying that the area of half-light ellipse A={pi}*Re2 (logMsRe) (phys.mass)
  log(Md<Re) [Msun] (n) Enclosed DM mass within a sphere of circularized effective radius Re which satisfying that the area of half-light ellipse A={pi}*Re2 (logMdRe) (phys.mass)

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(n) indicates a possible blank or NULL column(i)indexed column
  fDM<Re  (n) DM fraction within a sphere of effective radius which satisfying that the area of half-light ellipse A={pi}*Re2 (fdm_Re) (phys.mass;arith.ratio)
  logM/Ldyn [Msun/Lsun](n) Best-fitting dynamical mass-to-light ratio in M{sun}/L{sun} units (logMLdyn) (phys.composition.massLightRatio)
  Chi2  (n) The reduced chi2 of best-fitting model, values are scaled to account for effect of standard dev. of chi2 itself and it should be only used in comparison between models (chi2_dof) (stat.fit.chi2)
  Rh arcsec (n) Radius r1/2 of the 3D sphere which encloses half the total luminosity of the galaxy (rhalf_arcsec) (phys.angSize)
  log(Mt<Rh) [Msun] (n) Enclosed total stellar matter+DM+BH mass within a sphere of 3D half-light radius Rh (logMtrhalf) (phys.mass)
  log(Ms<Rh) [Msun] (n) Enclosed stellar matter mass within a sphere of 3D half-light radius Rh (logMsrhalf) (phys.mass)
  log(Md<Rh) [Msun] (n) Enclosed DM mass within a sphere of 3D half-light radius Rh (logMdrhalf) (phys.mass)
  GmwtRe  (n) Mass-weighted total density slope {Gamma}bart within a sphere of effective radius Re (MWGtRe) (spect.index;arith;meta.modelled)
  GmwsRe  (n) Mass-weighted stellar density slope {Gamma}bar* within a sphere of effective radius Re (MWGsRe) (spect.index;arith;meta.modelled)
  GmwdRe  (n) Mass-weighted DM density slope {Gamma}barDM within a sphere of effective radius Re (MWGsRe) (spect.index;arith;meta.modelled)
  GmwtRh  (n) Mass-weighted total density slope {Gamma}bart within a sphere of 3D half-light radius Rh (MWGtrhalf) (spect.index;arith;meta.modelled)
  GmwsRh  (n) Mass-weighted stellar density slope {Gamma}bar* within a sphere of 3D half-light radius Rh (MWGsrhalf) (spect.index;arith;meta.modelled)
  GmwdRh  (n) Mass-weighted DM density slope {Gamma}barDM within a sphere of 3D half-light radius Rh (MWGdrhalf) (spect.index;arith;meta.modelled)
  log(GavtRe) [-] (n) Average logarithmic total density slope {Gamma}t between 0.1 and 1 effective radius Re (Gt_Re) (spect.index;arith;meta.modelled)
  log(GavsRe) [-] (n) Average logarithmic stellar density slope {Gamma}* between 0.1 and 1 effective radius Re (Gs_Re) (spect.index;arith;meta.modelled)
  log(GavdRe) [-] (n) Average logarithmic DM density slope {Gamma}DM between 0.1 and 1 effective radius Re (Gd_Re) (spect.index;arith;meta.modelled)

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