chemical_abundances (ravedr4.chemical_abundances)
Description
The page describes the columns and properties of the table with abundances from C. Boeche"s pipeline.
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 |
|
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] |
|
teff_k | float | phys.temperature.effective | K |
Effective temperature |
logg_k | float | phys.gravity |
Log gravity (Note 2, DR5) |
|
met_n_k | float | phys.abund.Z |
Calibrated metallicity [m/H] |
|
met_c | float | phys.abund.Z |
[m/H] [Chemical Pipeline] |
|
alpha_c | float | phys.abund |
[Alpha/Fe] [Chemical pipeline] |
|
stn_c | float | stat.snr |
Signal / Noise Ratio Chemical pipeline |
|
frac_c | float | stat.value |
Chemical pipeline, fraction |
|
n_tot | short | meta.number |
total number of evaluated spectra |
|
chisq_c | float | stat.fit.chi2 |
chi square [Chemical pipeline] |
|
sigma_c | float | stat.param |
Chemical pipeline, best matching line profile |