VizieR

CfA VizieR . ADAC VizieR . Cambridge (UK) VizieR . IUCAA VizieR . INASAN VizieR .
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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/690/A125
  Gaia parallax uncertainties and RHD simulations (Beguin+, 2024)
ReadMe+ftp
2024A&A...690A.125B
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Post annotation 		img(gal)
1.J/A+A/690/A125/tablea1RHD simulation parameters (31 rows)
2.J/A+A/690/A125/tablea2(c)Parameters of the sample Miras (53 rows)
3.J/A+A/690/A125/tablea3(c)Stellar parameters of the Miras inferred from the simulations (53 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)Id  Model identification number (Note 1)   (meta.id)
  (1)Sim (char) Simulation name (meta.id;stat.fit)
  (1)M* Msun Stellar mass (phys.mass)
   (ALL)L* Lsun Average emitted luminosity (phys.luminosity)
  (1)R* Rsun Average approximate stellar radius (phys.size.radius;stat.mean)
  (1)Teff K Effective temperature (phys.temperature.effective)
  (1)logg [cm/s2] Surface gravity (phys.gravity)
  (1)tavg yr Stellar time used for the averaging of the rest of the quantities (time.epoch)
  (1)P d Pulsation period (time.period)
  (1)e_P d Pulsation period error (stat.error)

ALL cols		    
 (i)indexed column
  (1)Px au Time-averaged position Px (pos.cartesian.x;instr.det)
  (1)n_Px (char) [a] Note on Px (Note 2)   (meta.note)
  (1)Py au Time-averaged position Py (pos.cartesian.y;instr.det)
  (1)n_Py (char) [a] Note on Px (Note 2)   (meta.note)
  (1)sigP au Standard deviation of the photocentre displacement in AU (stat.stdev)
  (1)n_sigP (char) [a] Note on Px sigP (Note 2)   (meta.note)
  (1)sipPp  Standard deviation of the photocentre displacement in percentage of stellar radius (stat.stdev)
  (1)n_sipPp (char) [a] Note on Px (Note 2)   (meta.note)
  (2+3)Name (char) Miras' name (meta.id;meta.main)
  (2+3)Pobs d Pulsation period obtained from light curves (Note 1)   (time.period)
  (2+3)RUWE  RUWE (stat.error)
  (2+3)Nper  Number of visibility periods used in the astrometric solution (Note 2)   (meta.number)
  (2+3)Ngood  Total number of good observations along-scan (astrometricngoodobsal) by Gaia to compute the astrometric solution (meta.number)

ALL cols		    
 (i)indexed column
  (2+3)e_L* Lsun Negative luminosity uncertainty (stat.error)
  (2+3)E_L* Lsun Positive luminosity uncertainty (stat.error;stat.max)
  (2+3)plx mas Gaia DR3 parallax (pos.parallax.trig)
  (2+3)plxcorr mas Corrected Gaia DR3 parallax according to Lindegren et al. (2021A&A...649A...4L) (pos.parallax.trig)
  (2+3)e_plx mas Parallax uncertainty (stat.error;pos.parallax)
  (2+3)Pop (char) Population membership based on a study of stellar total space velocity according to Chen et al. (2021ApJ...909..115C), halo stars are more metal poor (meta.code)
  (2+3)Simbad (char) ask the Simbad data-base about this object (meta.ref.url)
  (2+3)_RA deg (i) Right Ascension (J2000) from SIMBAD (not part of the original data) (pos.eq.ra;meta.main)
  (2+3)_DE deg (i) Declination (J2000) from SIMBAD (not part of the original data) (pos.eq.dec;meta.main)
  (3)P10 d Pulsation period inferred from simulations at 1.0M☉ (time.period)
  (3)DP10 % Relative difference between Pobs and P10 (stat.fit.param)
  (3)P15 d Pulsation period inferred from simulations at 1.5M☉ (time.period)
  (3)DP15 % Relative difference between Pobs and P15 (stat.fit.param)

ALL cols		    
 (i)indexed column
  (3)logg10 [cm/s2] Surface gravity from simulations at 1.0M☉ (phys.gravity)
  (3)logg15 [cm/s2] Surface gravity from simulations at 1.5M☉ (phys.gravity)
  (3)R10 Rsun Radius inferred from simulations at 1.0M☉ (phys.size.radius)
  (3)R15 Rsun Radius inferred from simulations at 1.5M☉ (phys.size.radius)
  (3)Teff10 K Effective temperature from simulations at 1.0M☉ (phys.temperature.effective)
  (3)Teff15 K Effective temperature from simulations at 1.5M☉ (phys.temperature.effective)

ALL cols		    
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