RAVE DR5 stars, stellar parameters from Cannon (ravedr5.rave_on)
The table has 520701 rows, 58 columns.
Description
RAVE DR5 stars, stellar parameters from Cannon (Casey, 2016)
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 |
|
| raveid | char | meta.id |
(J2000 GCS), see Note in DR4 |
|
| radeg | double | pos.eq.ra | deg |
Right Ascension (J2000) |
| dedeg | double | pos.eq.dec | deg |
Declination (J2000) |
| hrv | float |
spect.dopplerVeloc pos.heliocentric |
km/s |
Heliocentric radial velocity |
| ehrv | float |
stat.error spect.dopplerVeloc pos.heliocentric |
km/s |
Error of Heliocentric radial velocity stat.error |
| stddev_hrv | double |
stat.stddev spect.dopplerVeloc pos.heliocentric |
km/s |
Standard deviation in HRV from 10 resampled spectra |
| mad_hrv | double |
stat.error stat.median |
km/s |
Mean absolute deviation in HRV from 10 resampled spectra |
| correlationcoeff | double | stat.correlation |
Tonry-Davis $R$ correlation coefficient |
|
| peakheight | double |
stat.correlation stat.value |
Height of correlation peak |
|
| peakwidth | double |
stat.correlation stat.value |
km/s |
Width of correlation peak |
| correctionrv | double |
spect.dopplerVeloc arith.zp |
km/s |
Zero point correction applied Heliocentric Radial Velocity |
| skyrv | double | spect.dopplerVeloc | km/s |
Measured HRV of sky |
| eskyrv | double |
stat.error spect.dopplerVeloc |
km/s |
error HRV of sky |
| skycorrelationcoeff | double | stat.correlation |
Correlation Coefficient |
|
| vrot_sparv | double | phys.veloc.rotat | km/s |
Rotational Velocity |
| zeropointflag | char | meta.code.qual |
Quality Flag for ZeroPoint correction (see DR3, Note ) |
|
| c1 | char | meta.code |
1.st minimum distance to base spectrum given by one of the types (enumeration [a,b,c,d,e,g,h,n,o,p,t,u,w]) |
|
| c2 | char | meta.code |
2.nd minimum distance to base spectrum given by one of the types (enumeration [a,b,c,d,e,g,h,n,o,p,t,u,w]) |
|
| c3 | char | meta.code |
3.rd minimum distance to base spectrum given by one of the types (enumeration [a,b,c,d,e,g,h,n,o,p,t,u,w]) |
|
| c4 | char | meta.code |
4.th minimum distance to base spectrum given by one of the types (enumeration [a,b,c,d,e,g,h,n,o,p,t,u,w]) |
|
| c5 | char | meta.code |
5.th minimum distance to base spectrum given by one of the types (enumeration [a,b,c,d,e,g,h,n,o,p,t,u,w]) |
|
| c6 | char | meta.code |
6.th minimum distance to base spectrum given by one of the types (enumeration [a,b,c,d,e,g,h,n,o,p,t,u,w]) |
|
| c7 | char | meta.code |
7.th minimum distance to base spectrum given by one of the types (enumeration [a,b,c,d,e,g,h,n,o,p,t,u,w]) |
|
| c8 | char | meta.code |
8.th minimum distance to base spectrum given by one of the types (enumeration [a,b,c,d,e,g,h,n,o,p,t,u,w]) |
|
| c9 | char | meta.code |
9.th minimum distance to base spectrum given by one of the types (enumeration [a,b,c,d,e,g,h,n,o,p,t,u,w]) |
|
| c10 | char | meta.code |
10.th minimum distance to base spectrum given by one of the types (enumeration [a,b,c,d,e,g,h,n,o,p,t,u,w]) |
|
| c11 | char | meta.code |
11.th minimum distance to base spectrum given by one of the types (enumeration [a,b,c,d,e,g,h,n,o,p,t,u,w]) |
|
| c12 | char | meta.code |
12.th minimum distance to base spectrum given by one of the types (enumeration [a,b,c,d,e,g,h,n,o,p,t,u,w]) |
|
| c13 | char | meta.code |
13.th minimum distance to base spectrum given by one of the types (enumeration [a,b,c,d,e,g,h,n,o,p,t,u,w]) |
|
| c14 | char | meta.code |
14.th minimum distance to base spectrum given by one of the types (enumeration [a,b,c,d,e,g,h,n,o,p,t,u,w]) |
|
| c15 | char | meta.code |
15.th minimum distance to base spectrum given by one of the types (enumeration [a,b,c,d,e,g,h,n,o,p,t,u,w]) |
|
| c16 | char | meta.code |
16.th minimum distance to base spectrum given by one of the types (enumeration [a,b,c,d,e,g,h,n,o,p,t,u,w]) |
|
| c17 | char | meta.code |
17.th minimum distance to base spectrum given by one of the types (enumeration [a,b,c,d,e,g,h,n,o,p,t,u,w]) |
|
| c18 | char | meta.code |
18.th minimum distance to base spectrum given by one of the types (enumeration [a,b,c,d,e,g,h,n,o,p,t,u,w] ) |
|
| c19 | char | meta.code |
19.th minimum distance to base spectrum given by one of the types (enumeration [a,b,c,d,e,g,h,n,o,p,t,u,w]) |
|
| c20 | char | meta.code |
20.th minimum distance to base spectrum given by one of the types (enumeration [a,b,c,d,e,g,h,n,o,p,t,u,w]) |
|
| teff | double | phys.temperature.effective | K |
Effective temperature, Casey et al. (2016) |
| logg | double | phys.gravity |
Log gravity, Casey et al. (2016) |
|
| fe_h | double | phys.abund.Z |
[Fe/H]; abundance of Fe, Casey et al. (2016) |
|
| o_h | double | phys.abund.Z |
[O/H]; abundance of O, Casey et al. (2016) |
|
| mg_h | double | phys.abund.Z |
[Mg/H]; abundance of Mg, Casey et al. (2016) |
|
| al_h | double | phys.abund.Z |
[Al/H]; abundance of Al, Casey et al. (2016) |
|
| si_h | double | phys.abund.Z |
[Si/H]; abundance of Si, Casey et al. (2016) |
|
| ca_h | double | phys.abund.Z |
[Ca/H]; abundance of Ca, Casey et al. (2016) |
|
| ni_h | double | phys.abund.Z |
[Ni/H]; abundance of Ni, Casey et al. (2016) |
|
| e_teff | double |
stat.error phys.temperature.effective |
K |
Eerror of effective temperature, Casey et al. (2016) |
| e_logg | double |
stat.error phys.gravity |
Error of log gravity, Casey et al. (2016) |
|
| e_fe_h | double |
stat.error phys.abund.Z |
Error of [Fe/H]; abundance of Fe, Casey et al. (2016) |
|
| e_o_h | double |
stat.error phys.abund.Z |
Error of [O/H]; abundance of O, Casey et al. (2016) |
|
| e_mg_h | double |
stat.error phys.abund.Z |
Error of [Mg/H]; abundance of Mg, Casey et al. (2016) |
|
| e_al_h | double |
stat.error phys.abund.Z |
Error of [Al/H]; abundance of Al, Casey et al. (2016) |
|
| e_si_h | double |
stat.error phys.abund.Z |
Error of [Si/H]; abundance of Si, Casey et al. (2016) |
|
| e_ca_h | double |
stat.error phys.abund.Z |
Error of [Ca/H]; abundance of Ca, Casey et al. (2016) |
|
| e_ni_h | double |
stat.error phys.abund.Z |
Error of [Ni/H]; abundance of Ni, Casey et al. (2016) |
|
| snr | double | stat.snr |
Signal/Noise Ratio, Casey et al. (2016) |
|
| r_chi_sq | double | stat.fit.chi2 |
chi square, Casey et al. (2016) |
|
| qc | short |
