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:
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NB: The epoch used for the query is the original epoch of the table(s)Radius Box size

  
J/PASJ/59/335
  Properties of 160 F-K disk dwarfs/subgiants (Takeda+, 2007)
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2007PASJ...59..335T
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1.J/PASJ/59/335/catalog(c)Results on program stars: astrophysical parameters, abundances, kinematic parameters (tables 1, E1, E2 and E3 of paper) (160 rows)
2.J/PASJ/59/335/mabundAverage abundances (from tablee3) (2552 rows)
3.J/PASJ/59/335/xhcorCorrections on the final (line-averaged) results of [ScII/H], [VI/H], [MnI/H] and [CoI/H] caused by inclusion of the hyper-fine splitting effect for each of the relevant lines (from tablee4) (569 rows)
4.J/PASJ/59/335/lgf*Wavelength and the loggf data of each hyper-fine splitting (hfs) component (from tablee4) (Note) (365 rows)
5.J/PASJ/59/335/difResults of abundance corrections caused by inclusion of the hyper-fine splitting (hfs) effect for the relevant line (from tablee4) (2824 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)
  (1)n_HD (char) [P] 'P' when star harbors planet(s) (meta.note)
   (1+2+3+5)HD  (i) HD number of the star (meta.id;meta.main)
  (1)HR  (n) HR number of the star (meta.id)
  (1)HIP  (n) HIP number of the star (meta.id)
  (1)HIP_data (char) Link to all parameters supplied by the results of the Hipparcos mission (phys.abund)
  (1)Name (char) Star name (meta.id)
  (1)SpType (char) MK spectral type (src.spType)
  (1+3+5)Teff K Effective temperature (Note 1)   (phys.temperature.effective)
  (1+3)logg [cm/s2] Surface gravity (Note 1)   (phys.gravity)
  (1+3+5)vt km/s Microturbulent velocity (Note 1)   (phys.veloc)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1+3)[Fe/H] [Sun] Metallicity (Note 1)   (phys.abund.Z)
  (1)logL [solLum] Stellar luminosity derived as -0.4(Mbol-4.75) (phys.luminosity)
  (1)Mass solMass Mass (Note 2)   (phys.mass)
  (1)logAge [yr] Age (Note 2)   (time.age)
  (1)q_logAge (char) [ABC] Quality flag showing the reliability of age (see Sect. 2.1 for more details) (Note 3)   (meta.code.qual;time.age)
  (1)V(LSR) km/s Space speed relative to the LSR (Note G1)   (phys.veloc)
  (1)Abun (char) Display the detailed abundance corrections with hyper-fine splitting (meta.ref.url)
  (1)Simbad (char) ask the Simbad data-base about this object
  (1)Teff2 K Effective temperature (Note 1)   (phys.temperature.effective)
  (1)logg2 [cm/s+2] logarithmic surface gravity (Note 1)   (phys.gravity)
  (1)vt2 km/s microturbulent velocity (Note 1)   (phys.veloc)
  (1)[Fe/H]2 [Sun] Fe abundance relative to the Sun (Note 1)   (phys.abund.Fe)
  (1)VMAG2 mag Absolute visual magnitude (Note 2)   (phys.magAbs;em.opt.V)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1)BC2 mag Bolometric correction (Note 2)   (phot.mag.bc)
  (1)Mbol2 mag Bolometric magnitude (Note 2)   (phot.mag.bol)
  (1)logL2 [solLum] logarithmic luminosity (phys.luminosity)
  (1)M(trk) solMass Stellar mass derived from evolutionary track (Note 3)   (phys.mass)
  (1)E_M(trk) solMass Possible error in M(trk) on the upper side (stat.error;stat.max)
  (1)e_M(trk) solMass Possible error in M(trk) on the lower side (stat.error)
  (1)M(iso) solMass Stellar mass derived from isochrones (phys.mass)
  (1)logg(TLM) [cm/s+2] Theorerical logg derived from Teff, L, and M(trk) (phys.gravity)
  (1)logAge(trk) [yr] log(stellar age) derived from evolutionary track (Note 3)   (arith.zp)
  (1)E_logAge(trk) [yr] Possible error in logAge(trk) on the upper side (stat.error;stat.max)
  (1)e_logAge(trk) [yr] Possible error in logAge(trk) on the lower side (stat.error)
  (1)q_logAge(trk) (char) Reliability of age(trk) (Note 4)   (meta.code.qual)
  (1)logAge(iso) [yr] log(stellar age) derived from isochrones (arith.zp)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1)PapII (char) Show the stellar parameters from PaperII (2005, Cat. J/PASJ/57/27) (meta.ref.url)
  (1)RAJ2000 "h:m:s" (i) Right ascension (J2000, Ep=1991.25, HIP) (pos.eq.ra;meta.main)
  (1)DEJ2000 "d:m:s" (i) Declination (J2000, Ep=1991.25, HIP) (pos.eq.dec;meta.main)
  (1)plx mas Parallax (Note 1)   (pos.parallax.trig)
  (1)pmRA mas/yr Proper motion in alpha direction (Note 1)   (pos.pm;pos.eq.ra)
  (1)pmDE mas/yr Proper motion in delta direction (Note 1)   (pos.pm;pos.eq.dec)
  (1)HRV km/s Heliocentric radial velocity (from table 2 of Paper I, Cat. J/PASJ/57/13) (spect.dopplerVeloc;pos.heliocentric)
  (1)Rm kpc Mean galactocentric distance (pos.distance;src.orbital)
  (1)zm kpc Maximum separation from the galactic plane (src.orbital)
  (1)e  Galactocentric orbital eccentricity (src.orbital.eccentricity;pos.galactocentric)
  (1)Ulsr km/s Space velocity in radial direction relative to LSR (phys.veloc;pos.cartesian.x)
  (1)Vlsr km/s Space velocity in tangential direction relative to LSR (phys.veloc;pos.cartesian.y)
  (1)Wlsr km/s Space velocity in vertical direction relative to LSR (phys.veloc;pos.cartesian.z)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1)PapI (char) Show tables from PaperI (2005, Cat. J/PASJ/57/13) for this star (meta.ref.url)
  (1)[Na/H] [Sun] Na abundance relative to the Sun (phys.abund)
  (1)[Mg/H] [Sun] Mg abundance relative to the Sun (MgI 8806 fit) (phys.abund)
  (1)[Al/H] [Sun] (n) Al abundance relative to the Sun (phys.abund)
  (1)[Si/H] [Sun] Si abundance relative to the Sun (phys.abund)
  (1)[S/H] [Sun] (n) S abundance relative to the Sun (SI 8684 fit) (phys.abund)
  (1)[Ca/H] [Sun] Ca abundance relative to the Sun (phys.abund)
  (1)[ScI/H] [Sun] (n) Sc abundance relative to the Sun (from ScI) (phys.abund)
  (1)[ScII/H] [Sun] Sc abundance relative to the Sun (from ScII) (phys.abund)
  (1)[TiI/H] [Sun] Ti abundance relative to the Sun (from TiI) (phys.abund)
  (1)[TiII/H] [Sun] Ti abundance relative to the Sun (from TiII) (phys.abund)
  (1)[VI/H] [Sun] (n) V abundance relative to the Sun (from VI) (phys.abund)
  (1)[VII/H] [Sun] (n) V abundance relative to the Sun (from VII) (phys.abund)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1)[CrI/H] [Sun] Cr abundance relative to the Sun (from CrI) (phys.abund)
  (1)[CrII/H] [Sun] Cr abundance relative to the Sun (from CrII) (phys.abund)
  (1)[Mn/H] [Sun] (n) Mn abundance relative to the Sun (phys.abund)
  (1)[Co/H] [Sun] Co abundance relative to the Sun (phys.abund)
  (1)[Ni/H] [Sun] Ni abundance relative to the Sun (phys.abund)
  (1)[Cu/H] [Sun] (n) Cu abundance relative to the Sun (phys.abund)
  (1)[Zn/H] [Sun] (n) Zn abundance relative to the Sun (phys.abund)
  (1)A(Mg)  Mg abundance from 8806 fit (normalisation of H=12.00) (phys.abund)
  (1)EW(Mg) 0.1pm EW(MgI 8806.8) inversely computed from A(Mg) (spect.line.eqWidth;meta.modelled)
  (1)A(S)  S abundance from 8693-5 fit (normalisation of H=12.00) (phys.abund)
  (1)EW(S1) 0.1pm (n) EW(SI 8693.1) inversely computed from A(S) (spect.line.eqWidth;meta.modelled)
  (1)EW(S2) 0.1pm (n) EW(SI 8693.9) inversely computed from A(S) (spect.line.eqWidth;meta.modelled)
  (1)EW(S3) 0.1pm (n) EW(SI 8694.6) inversely computed from A(S) (spect.line.eqWidth;meta.modelled)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2)Nline  Number of lines for the species (meta.number)
  (2+3+4+5)Ion  Ion code (Note G2)   (meta.code;phys.atmol.ionStage)
  (2)o_<delA>  Number of lines actually adopted for computing the averaged abundances (meta.number)
  (2)<delA>  Average differential abundance (star-Sun) (phys.abund)
  (2)e_<delA>  rms uncertainty on <delA> (stat.error)
  (2)FileName (char) Name of the file with individual measurements in subdirectory cmb (meta.id;meta.file)
  (3)[X/H](hfs)  final [X/H] value obtained with hfs (phys.abund)
  (3)[X/H](nohf)  final [X/H] value obtained without hfs (phys.abund)
  (3+5)delta  hfs correction ([X/H](hfs)-[X/H](nohf)) (phys.abund)
  (4+5)lambda 0.1nm Line wavelength (em.wl;spect.line)
  (4)o_Ion  Number of hyperfine components (meta.number)
  (4)lam.hf 0.1nm Wavelength of the hyperfine components (em.wl)
  (4)chi eV (n) lower excitation potential (phys.atmol.excitation;stat.min)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (4)loggf  log of (statistical weight times oscillator strength) (arith.zp)
  (5)logg [m/s2] Logarithmic surface gravity (phys.gravity)
  (5)[Fe/H]  Fe abundance relative to the Sun (phys.abund.Fe)
  (5)EW 0.1pm Equivalent width of the line (spect.line.eqWidth)
  (5)A(hfs)  Abundance obtained with hyperfine splitting (phys.abund)
  (5)A(nohf)  Abundance obtained without hyperfine splitting (phys.abund)

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