Distances RAVE DR5 (ravedr5.distances_pjm2017)
The table has 219565 rows, 99 columns.
Description
Distances 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) sprintf("J%02d%02d%04.1f%s%02d%02d%02d", $RA_h, $RA_m,(int(10*$RA_s+0.51))/10.0, $DEsign,$DE_h,$DE_m,int($DE_s+0.51)) RA(hh:mm:ss) Dec(hh:mm:ss) from fits file (Object ID (RA-DEC)) |
|
| radeg | double | pos.eq.ra | deg |
Right Ascension (J2000) |
| dedeg | double | pos.eq.dec | deg |
Declination (J2000) |
| glon | double | pos.galactic.lon | deg |
Longitude (J2000 GCS) |
| glat | double | pos.galactic.lat | deg |
Latitude (J2000 GCS) |
| 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 |
| pmra_tgas | double |
pos.pm pos.eq.ra |
mas/yr |
Proper motion (Right Ascension) |
| pmra_error_tgas | double |
stat.errror pos.pm pos.eq.ra |
mas/yr |
Error of proper motion (RA) |
| pmde_tgas | double |
pos.pm pos.eq.dec |
mas/yr |
Proper motion (Declination) |
| pmde_error_tgas | double |
stat.error pos.pm pos.eq.dec |
mas/yr |
Error of proper motion (DE) |
| distance | float | pos.distance | pc |
spectrophotometric Distance (Binney et al. 2014) |
| edistance | float | pos.distance | pc |
Error of spectrophotometric Distance (Binney et al. 2014) |
| age | float | time.age | log10(age(yr)) |
Age estimation |
| eage | float |
arith stat.error |
yr |
Error Age estimation. |
| mass | float | phys.mass | solMass |
Mass |
| e_mass | float |
stat.error phys.mass |
solMass |
Error of Mass |
| 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 |
Error of spectrophotometric Parallax (Binney et al. 2014) |
| dist_mod | float | phot.mag.distMod | mag |
Distance Modulus from McMillan et al. 2017 |
| edist_mod | float | phot.mag.distMod | mag |
Error of distance Modulus from McMillan et al. 2017 |
| teff_pjm | double | phys.temperature.effective | K |
Effective temperature from reverse pipeline (McMillan et al 2017) |
| eteff_pjm | double | phys.temperature.effective | K |
Error effective temperature from reverse pipeline (McMillan et al 2017) |
| logg_pjm | double | phys.gravity |
Log gravity from reverse pipeline (McMillan et al 2017) |
|
| elogg_pjm | double | phys.gravity |
Log gravity from reverse pipeline (McMillan et al 2017) |
|
| 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 | stat.fit.param |
Property of multi-Gaussian distance modulus fit, see Section 9, eq. 5 |
|
| fitquality_gauss | float | meta.code.qual |
Given by symbol F in eq. 5 of McMillan et al. 2017 |
|
| fit_flag_gauss | int | meta.code.qual |
See paragraph 2.1 (McMillan et al. 2017) |
|
| av_schlegel | double | phys.absorption | mag |
Total Extinction in V-band from Schlegel et al. (1998) |
| logg_n_k | double | phys.gravity |
Log gravity (Note 2, DR5) |
|
| elogg_k | double | phys.gravity |
Log gravity (Note 2, DR5) |
|
| teff_ir | float | phys.temperature.effective | K |
Effective temperature from infrared flux method |
| eteff_ir | float |
stat.error phys.temperature.effective |
K |
Error of effective temperature from infrared flux method |
| met_n_k | double | phys.abund.Z |
Calibrated metallicity [m/H] |
|
| emet_k | double | phys.abund.Z |
Error of [m/H] |
|
| parallax_tgas | double | pos.parallax | mas |
Parallax |
| parallax_error_tgas | double |
stat.error pos.parallax |
mas |
Error of parallax |
| jmag_2mass | float |
phot.mag em.IR.J |
mag |
J selected default magnitude from 2MASS |
| ejmag_2mass | float |
stat.error phot.mag em.IR.J |
mag |
error 2MASS J magnitude |
| hmag_2mass | float |
phot.mag em.IR.H |
mag |
H selected default magnitude from 2MASS |
| ehmag_2mass | float |
stat.error phot.mag em.IR.H |
mag |
error 2MASS H magnitude |
| kmag_2mass | float |
phot.mag em.IR.K |
mag |
K selected default magnitude from 2MASS |
| ekmag_2mass | float |
stat.error phot.mag em.IR.K |
mag |
error 2MASS K magnitude |
| w1mag_allwise | float |
phot.mag em.opt |
mag |
W1 magnitude from ALLWISE |
| ew1mag_allwise | float |
stat.error phot.mag em.opt |
mag |
Error W1 magnitude from ALLWISE |
| w2mag_allwise | float |
phot.mag em.opt |
mag |
W2 magnitude from ALLWISE |
| ew2mag_allwise | float |
stat.error phot.mag em.opt |
mag |
Error W2 magnitude from ALLWISE |
| 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] |
|
| 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]) |
|
| snr | double | stat.snr |
Signal/Noise Ratio, Casey et al. (2016) |
|
| algo_conv_k | short | meta.code.qual |
Quality Flag for Stellar Parameter pipeline,[0..4] |
|
| flag_lowlogg | short | meta.code.qual |
0 => logg >= 2.0, 1 => logg <2.0 |
|
| flag_outlier | short | meta.code.qual |
0 => not outlier, 1 => outlier (TGAS & RAVE-only differ by more than 4 sigma |
|
| flag_n | short | meta.code.qual |
0 => spectrum flagged as normal by first 3 labels from Matijevič et al (2012, ApJS, 200, 14), 1 => spectrum flagged as normal |
|
| flag_pole | short | meta.code.qual |
0 => good TGAS region, 1 => source lies in problematic TGAS region near ecliptic pole (165 < lambda <195, beta < 30), see McMillan et al. 2017 |
|
| flag_dup | short | meta.code.qual |
0 => only/best spectrum of start in RAVEDR5, 1 => spectrum of same star with higher SNR is in RAVEDR5 |
|
| flag_any | short | meta.code.qual |
0 => all five flags above are 0, 1 => any of the above flags are 1 |
