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J/MNRAS/515/1903
  Stars cluster and RGBs study in NGC362 (Vargas+, 2022)
ReadMe+ftp
2022MNRAS.515.1903V
Similar Catalogs
Post annotation 		img(gal)
1.J/MNRAS/515/1903/table(c)*Chromosome map of NGC0362 with HST photometry (Note) (1172 rows)
2.J/MNRAS/515/1903/table1(c)Gaia and HST astrometric and photometric data for the 12 target stars (12 rows)
3.J/MNRAS/515/1903/table2Atmospheric parameters for the 11 target stars derived with isochrone fits (11 rows)
4.J/MNRAS/515/1903/table3Atmospheric parameters for the 11 target stars derived with Marino and Mott methods (11 rows)
5.J/MNRAS/515/1903/table4Parameters and metallicities obtained spectroscopically using the FeI and FeII lines (11 rows)

Simple ConstraintList Of Constraints
 
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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)ID  Star identifier number (ID) (meta.id;meta.main)
  (1+2)RAJ2000 deg (i) Right ascension (J2000) at Ep=2015.0 from HUGS Catalog (2015AJ....149...91P) (RA) (pos.eq.ra;meta.main)
  (1+2)DEJ2000 deg (i) Declination (J2000) at Ep=2015.0 from HUGS Catalog (2015AJ....149...91P) (DEC) (pos.eq.dec;meta.main)
  (1+2)F275Wmag mag Apparent magnitude in F275W HST filter from UV Legacy Survey Nardiello et al. (2018MNRAS.481.3382N) (F275W) (phot.mag;em.UV.200-300nm)
  (1+2)F336Wmag mag Apparent magnitude in F336W HST filter from UV Legacy Survey Nardiello et al. (2018MNRAS.481.3382N) (F336W) (phot.mag;em.opt.U)
  (1+2)F438Wmag mag Apparent magnitude in F438W HST filter from UV Legacy Survey Nardiello et al. (2018MNRAS.481.3382N) (F438W) (phot.mag;em.opt.B)
  (1+2)F814Wmag mag Apparent magnitude in F814W HST filter from UV Legacy Survey Nardiello et al. (2018MNRAS.481.3382N) (F814W) (phot.mag;em.opt.I)
  (1)F275W-F814W mag Delta(F275W,F814W) pseudo-colour (|F275W-F814W|) (phot.mag;arith.diff;em.UV.200-300nm)
  (1)C mag Delta(CF275W,F336W,F438W) pseudo-colours as (F275W-F336W) - (F336W-F438W) (DeltaCF275W,F336W,F438W) ((unassigned);pos.distance.component;em.UV.200-300nm)
  (1)GaiaDR3 (char) Display the GaiaDR3 Cat. I/355 (meta.ref.url)

ALL cols		    
 (i)indexed column
  (2)pmRA mas/yr Proper motions in right ascension direction (pmRA*cosDE) from Gaia eDR3 (pmRA) (pos.pm;pos.eq.ra)
  (2)pmDE mas/yr Proper motion in declination direction from Gaia eDR3 (pmDEC) (pos.pm;pos.eq.dec)
  (2)Vmag mag Apparent magnitude in optical V band based on F438W, F606W and F814W HST filters (V) (phot.mag;em.opt.V;arith)
  (2)Gmag mag G-band mean magnitude (Vega) from Gaia DR2 (G) (phot.mag;stat.mean;em.opt)
  (2)BPmag mag Integrated BP mean magnitude (Vega) from Gaia DR2 (Bp) (phot.mag;stat.mean;em.opt.B)
  (2)RPmag mag Integrated RP mean magnitude (Vega) from Gaia DR2 (Rp) (phot.mag;em.opt.R)
  (2)F606Wmag mag Apparent magnitude in F606W HST filter from UV Legacy Survey Nardiello et al. (2018MNRAS.481.3382N) (F606W) (phot.mag;em.opt.R)
  (2)RV km/s Spectroscopic heliocentric radial velocity from MIKE spectrograph as explained in the section 3 (RVhelio) (spect.dopplerVeloc;pos.heliocentric;obs)
  (2)_RA.icrs deg (i) Right Ascension (ICRS, epoch 2000) computed by CDS (pos.eq.ra)
  (2)_DE.icrs deg (i) Declination (ICRS, epoch 2000) computed by CDS (pos.eq.dec)
  (3)TeffGaiam11 K Effective temperature obtained via 11 Gyr isochrone fitting using Gaia data (TGAIAm11) (phys.temperature.effective;meta.modelled)
  (3)loggGaiam11 [cm/s2] Logarithm of the surface gravity obtained via 11 Gyr isochrone fitting using Gaia data (gGAIAm11) (phys.gravity;meta.modelled)
  (3)TeffGaiam09 K Effective temperature obtained via 9 Gyr isochrone fitting using Gaia data (TGAIAm09) (phys.temperature.effective;meta.modelled)

ALL cols		    
 (i)indexed column
  (3)loggGaiam09 [cm/s2] Logarithm of the surface gravity obtained via 9 Gyr isochrone fitting using Gaia data (gGAIAm09) (phys.gravity;meta.modelled)
  (3)TeffHSTm11 K Effective temperature obtained via 11 Gyr isochrone fitting using HST data (THSTm11) (phys.temperature.effective;meta.modelled)
  (3)loggHSTm11 [cm/s2] Logarithm of the surface gravity obtained via 11 Gyr isochrone fitting using HST data (gHSTm11) (phys.gravity;meta.modelled)
  (3)TeffHSTm09 K Effective temperature obtained via 9 Gyr isochrone fitting using HST data (THSTm09) (phys.temperature.effective;meta.modelled)
  (3)loggHSTm09 [cm/s2] Logarithm of the surface gravity obtained via 9 Gyr isochrone fitting using HST data (gHSTm09) (phys.gravity;meta.modelled)
  (3)loggphot [cm/s2] Logarithm of the surface gravity obtained with the canonical relation as the described in section 4 (loggphot) (phys.gravity;meta.modelled)
  (3+4+5)Teff K Effective temperature used to compute vt and [Fe/H] (Teff) (phys.temperature.effective;meta.modelled)
  (3+4+5)logg [cm/s2] Logarithm of the surface gravity used to compute vt and [Fe/H] (logg) (phys.gravity;meta.modelled)
  (3+5)Vt km/s Microturbulent velocity obtained assuming Teff, log(g) and FeI line spectra (vt) (phys.veloc.microTurb;meta.modelled)
  (3+4+5)[Fe/H] [Sun] Iron to hydrogen abundance ratio assuming Teff, log(g) and FeI line spectra ([Fe/H]) (phys.abund.Fe;arith.ratio;meta.modelled)
  (3)[FeII/H] [Sun] Derived ionic iron FeII to hydrogen abundance ratio ([FeII/H]) (phys.abund.Fe;arith.ratio;meta.modelled)
  (3+4+5)Class (char) [a/n] Star classification a for anomalous and n for normal (Class) (src.class)
  (4)VtMott km/s Microturbulence velocity (vtMott) (Note 1)   (phys.veloc.microTurb;meta.modelled)

ALL cols		    
 (i)indexed column
  (4)VtMarino km/s Microturbulence obtained from empirical relation in Marino et al. 2008A&A...490..625M, Cat. J/A+A/490/625 (vtMarino) (phys.veloc.microTurb;meta.modelled)

ALL cols		    
 (i)indexed column
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