RAVE Gravity calibration (ravedr5.rave_gravity_sc)

The table has 262510 rows, 43 columns.

Description

Gravity from seismic calibrations (Valentini) with RAVE DR5 data


Change History:

08.11.2016:

rows added for syncing with RAVE_DR5


Attribution

Funding for Rave has been provided by:

  • the Leibniz Institute for Astrophysics Potsdam (AIP);
  • the Australian Astronomical Observatory;
  • the Australian National University;
  • the Australian Research Council;
  • the French National Research Agency;
  • the German Research Foundation (SPP 1177 and SFB 881);
  • the European Research Council (ERC-StG 240271 Galactica);
  • the Istituto Nazionale di Astrofisica at Padova;
  • the Johns Hopkins University;
  • the National Science Foundation of the USA (AST-0908326);
  • the W. M. Keck foundation;
  • the Macquarie University;
  • the Netherlands Research School for Astronomy;
  • the Natural Sciences and Engineering Research Council of Canada;
  • the Slovenian Research Agency;
  • the Swiss National Science Foundation;
  • the Science & Technology FacilitiesCouncil of the UK;
  • Opticon;
  • Strasbourg Observatory;
  • the Universities of Basel, Groningen, Heidelberg and Sydney.

This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the GaiaData Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement.

Columns

Name Type UCD Unit Description
rave_obs_id char meta.id

Unique Identifier for RAVE objects, Observation Date, Fieldname, Fibernumber

logg_sc float phys.gravity

Log gravity calibrated asteroseismically (V16)

elogg_sc float phys.gravity

Error of Log gravity calibrated asteroseismically (V16)

flag050 short meta.code

Difference between logg MV and logg K is less than 0.5 dex. 0=false 1= true

flag075 short meta.code

Difference between logg MV and logg K is less than 0.75 dex. 0=false 1= true

flag_m short meta.code

Normal star, meaning c1 - c20 are all "n". 0=false 1= true

teff_ir double phys.temperature.effective K

Effective temperature from infrared flux method

mg float phys.abund.Z

[Mg/H] abundance of Mg

mg_n short meta.number

Number of used spectral lines in calc. of [Mg/H]

al float phys.abund.Z

[Al/H] abundance of Al

al_n short meta.number

Number of used spectral lines in calc. of [Al/H]

si float phys.abund.Z

[Si/H] abundance of Si

si_n short meta.number

Number of used spectral lines in calc. of [Si/H]

ti float phys.abund.Z

[Ti/H] abundance of Ti

ti_n short meta.number

Number of used spectral lines in calc. of [Ti/H]

fe float phys.abund.Z

[Fe/H] abundance of Fe

fe_n short meta.number

Number of used spectral lines in calc. of [Fe/H]

ni float phys.abund.Z

[Ni/H] abundance of Ni

ni_n short meta.number

Number of used spectral lines in calc. of [Ni/H]

alpha_c float phys.abund

[Alpha/Fe] [Chemical pipeline]

chisq_c float stat.fit.chi2

chi square [Chemical pipeline]

frac_c float stat.value

Fraction of spectrum used [Chemical pipeline]

av_schlegel double phys.absorption mag

Total Extinction in V-band from Schlegel et al. (1998)

distance float pos.distance kpc

spectrophotometric Distance (Binney et al. 2014)

edistance float pos.distance kpc

Error of spectrophotometric Distance (Binney et al. 2014)

log_av float phys.absorption

log_10(Av) optical extinction, see p4 ff, Mon. Not. R. Astron. Soc. 000, 1-8 (2012)

elog_av float stat.error
phys.absorption

Error of log_10(Av) optical extinction, see p4 ff, Mon. Not. R. Astron. Soc. 000, 1-8 (2012)

parallax float pos.parallax mas

Parallax

eparallax float stat.error
pos.parallax
mas
distancemodulus_binney float phot.mag.distMod mag

Distance Modulus from Binney et al. 2014

edistancemodulus_binney float phot.mag.distMod mag

Error of distance Modulus from Binney et al. 2014

fit_flag_binney int meta.code.qual

See final paragraph 3 of Binney et al. (2014)

fitquality_binney float meta.code.qual

Given by symbol F in eq 15 of Binney et al. (2014)

n_gauss_fit int meta.number

Number of components required for multi-aussian distance modulus fit

gauss_mean_1 float stat.fit.param

Property of multi-Gaussian distance modulus fit, see Section 9, eq. 5

gauss_sigma_1 float stat.fit.param

Property of multi-Gaussian distance modulus fit, see Section 9, eq. 5

gauss_frac_1 float stat.fit.param

Property of multi-Gaussian distance modulus fit, see Section 9, eq. 5

gauss_mean_2 float stat.fit.param

Property of multi-Gaussian distance modulus fit, see Section 9, eq. 5

gauss_sigma_2 float stat.fit.param

Property of multi-Gaussian distance modulus fit, see Section 9, eq. 5

gauss_frac_2 float stat.fit.param

Property of multi-Gaussian distance modulus fit, see Section 9, eq. 5

gauss_mean_3 float stat.fit.param

Property of multi-Gaussian distance modulus fit, see Section 9, eq. 5

gauss_sigma_3 float stat.fit.param

Property of multi-Gaussian distance modulus fit, see Section 9, eq. 5

gauss_frac_3 float