VizieR

CfA VizieR . ADAC VizieR . Cambridge (UK) VizieR . IUCAA VizieR . INASAN VizieR .

VizieR

Simple TargetList Of TargetsFast Xmatch with large catalogs or Simbad
Target Name (resolved by Sesame) or Position:
Target dimension:
NB: The epoch used for the query is the original epoch of the table(s)Radius Box size

  
J/A+A/677/A143
  Angular momentum in MAGIC. I. Environment (Mercier+, 2023)
Post annotation
img(gal)
1.J/A+A/677/A143/tablee1Parameters for the kinematics sample (182 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) MUSE galaxy ID (Note 1)   (meta.id;meta.main)
  z  Spectroscopic systemic redshift derived from kinematics (src.redshift)
  RAJ2000 deg (i) Right Ascension of morphological centre (J2000) (pos.eq.ra;meta.main)
  DEJ2000 deg (i) Declination of morphological centre (J2000) (pos.eq.dec;meta.main)
  N  (n) Richness (i.e. number of galaxies) in the structure the galaxy belongs to (src.class.richness)
  R/R200  (n) Ratio of the projected distance of a galaxy to its host group's centre with its host group's radius. Field galaxies have a value of -99 (pos.distance;arith.ratio)
  dV/sigma  (n) Ratio of the systemic velocity of the galaxy along the line-of-sight with its host group's velocity dispersion. Field galaxies have a value of -99 (phys.veloc)
  Eta  (n) Environmental tracer combining R/R200 and dV/sigma (stat.fit.param)
  logOverDens  Log10 of the over-density around galaxies as measured by the VMC technique (phys.density;arith.ratio)
  logjHSTMM [kpc.km/s]Log10 of the specific stellar angular momentum derived from HST images and a mass model rotation curve (phys.angMomentum)
  logjHSTflat [kpc.km/s]Log10 of the specific stellar angular momentum derived from HST images and a flat model rotation curve (phys.angMomentum)
  logjexpMM [kpc.km/s]Log10 of the specific stellar angular momentum derived from an exponential mass distribution and a mass model rotation curve (phys.angMomentum)
  logjexpflat [kpc.km/s]Log10 of the specific stellar angular momentum derived from an exponential mass distribution and a flat model rotation curve (phys.angMomentum)
  GasDisp km/s Average ionised gas dispersion with LSF and beam-smearing corrections applied (arith.factor;instr.dispersion;stat.mean)
  logM* [Msun] Stellar mass within R22=2.2*Rd, with Rd the stellar disk scale length (phys.mass)

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(n) indicates a possible blank or NULL column(i)indexed column
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