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 Australian Astronomical Observatory; the Leibniz-Institut für Astrophysik Potsdam (AIP); 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 Facilities Council of the UK; Opticon; Strasbourg Observatory; and the Universities of Groningen, Heidelberg and Sydney. Based on data products from observations made with ESO Telescopes at the La Silla Paranal Observatory under programme ID 188.B3002.
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 |