Distances for RAVE DR5 (ravedr5.distancesnotgas_pjm2017)
The table has 224837 rows, 99 columns.
Description
Distances for RAVE DR5 sources which do not have TGAS parallaxes (see McMillan et al 2017)
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) |
| 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 (McMillan et al. 2017) |
| edistance | float | pos.distance | pc |
Error of spectrophotometric Distance (McMillan et al. 2017) |
| age | float |
arith stat.error |
yr |
Age estimation. |
| eage | float |
arith stat.error |
yr |
Error Age estimation. |
| mass | float | phys.mass | solMass |
Mass |
| e_mass | float | phys.mass | solMass |
Error Mass |
| log_av | float |
stat.error phys.absorption |
log_10(Av) optical extinction. See McMillan et al 2017, §2.1 |
|
| elog_av | float |
stat.error phys.absorption |
Error of log_10(Av) optical extinction. . See McMillan et al 2017, §2.1 |
|
| parallax | float | pos.parallax | mas |
spectrophotometric Parallax (McMillan et al. 2017) |
| eparallax | float |
stat.error pos.parallax |
mas |
Error of spectrophotometric Parallax (McMillan et al. 2017) |
| 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 McMillan et al. 2017, eq. 4 |
|
| gauss_sigma_1 | float | stat.fit.param |
Property of multi-Gaussian distance modulus fit, see McMillan et al. 2017, eq. 4 |
|
| gauss_frac_1 | float | stat.fit.param |
Property of multi-Gaussian distance modulus fit, see McMillan et al. 2017, eq. 4 |
|
| gauss_mean_2 | float | stat.fit.param |
Property of multi-Gaussian distance modulus fit, see McMillan et al. 2017, eq. 4 |
|
| gauss_sigma_2 | float | stat.fit.param |
Property of multi-Gaussian distance modulus fit, see McMillan et al. 2017, eq. 4 |
|
| gauss_frac_2 | float | stat.fit.param |
Property of multi-Gaussian distance modulus fit, see McMillan et al. 2017, eq. 4 |
|
| gauss_mean_3 | float | stat.fit.param |
Property of multi-Gaussian distance modulus fit, see McMillan et al. 2017, eq. 4 |
|
| gauss_sigma_3 | float | stat.fit.param |
Property of multi-Gaussian distance modulus fit, see McMillan et al. 2017, eq. 4 |
|
| gauss_frac_3 | float | stat.fit.param |
Property of multi-Gaussian distance modulus fit, see McMillan et al. 2017, eq. 4 |
|
| 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 of Kordopatis Pipeline |
|
| 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 |
