Seismic calibrated stellar parameters (ravedr6.dr6_seismic)
The table has 130501 rows, 22 columns.
Description
The table contains the asteroseismically calibrated red giant catalog. The calibration procedure is as outlined in DR5, but uses teff_irfm (see tablen dr6_irfm) as the prior for the effective temperature. (see RAVE DR5 II)
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; and 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 | |
chisq_sc | float | stat.fit.chi2 | chi square from seismic calibration | |
teff_sc | double | phys.temperature.effective | K | Effective temperature from seismic calibration |
teff_error_sc | float |
stat.error phys.temperature.effective |
K | Error of effective temperature from seismic calibration |
logg_sc | float | phys.gravity | dex | Log gravity |
logg_error_sc | float |
stat.error phys.gravity |
dex | Error of log gravity |
m_h_sc | float | phys.abund.Z | dex | Abundance |
m_h_error_sc | float |
stat.error phys.abund.Z |
dex | Error of abundance |
fe_h_sc | float | phys.abund.Z | dex | [Fe/H]; abundance of Fe |
fe_h_error_sc | float |
stat.error phys.abund.Z |
dex | Error of abundance of Fe |
mg_h_sc | float | phys.abund.Z | dex | [Mg/H]; abundance of Mg |
mg_h_error_sc | float |
stat.error phys.abund.Z |
dex | Error of abundance of Mg |
al_h_sc | float | phys.abund.Z | dex | [Al/H]; abundance of Al |
al_h_error_sc | float |
stat.error phys.abund.Z |
dex | Error of abundance of Al |
si_h_sc | float | phys.abund.Z | dex | [Si/H]; abundance of Si |
si_h_error_sc | float |
stat.error phys.abund.Z |
dex | Error of abundance of Si |
ca_h_sc | float | phys.abund.Z | dex | [Ca/H]; abundance of Ca |
ca_h_error_sc | float |
stat.error phys.abund.Z |
dex | Error of abundance of Ca |
ti_h_sc | float | phys.abund.Z | dex | [Ti/H]; abundance of Ti |
ti_h_error_sc | float |
stat.error phys.abund.Z |
dex | Error of abundance of Ti |
ni_h_sc | float | phys.abund.Z | dex | [Ni/H]; abundance of Ni |
ni_h_error_sc | float |
stat.error phys.abund.Z |
dex | Error of abundance of Ni |