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