Distances_PJM2017

Description

Distances for RAVE DR5 sources with TGAS parallaxes (see McMillan et al 2017)

The data can be accessed using the query interface or downloaded at Downloads. Please cite this data set using the unique digital object identifier doi:10.17876/rave/dr.5/033.

Columns

ColumnTypeUCDUnitDescription
RAVE_OBS_IDcharmeta.idUnique Identifier for RAVE objects, Observation Date, Fieldname, Fibernumber
RAVEIDcharmeta.id(J2000 GCS), see Note in DR4
RAdegdoublepos.eq.radegRight Ascension (J2000)
DEdegdoublepos.eq.decdegDeclination (J2000)
Glondoublepos.galactic.londegLongitude (J2000 GCS)
Glatdoublepos.galactic.latdegLatitude (J2000 GCS)
HRVfloatspect.dopplerVeloc
pos.heliocentric
km/sHeliocentric radial velocity
eHRVfloatstat.error
spect.dopplerVeloc
pos.heliocentric
km/sError of Heliocentric radial velocity stat.error
pmRA_TGASdoublepos.pm
pos.eq.ra
mas/yrProper motion (Right Ascension)
pmRA_error_TGASdoublestat.errror
pos.pm
pos.eq.ra
mas/yrError of proper motion (RA)
pmDE_TGASdoublepos.pm
pos.eq.dec
mas/yrProper motion (Declination)
pmDE_error_TGASdoublestat.error
pos.pm
pos.eq.dec
mas/yrError of proper motion (DE)
distancefloatpos.distancepcspectrophotometric Distance (McMillan et al. 2017)
edistancefloatpos.distancepcError of spectrophotometric Distance (McMillan et al. 2017)
agefloatarith
stat.error
yrAge estimation.
eagefloatarith
stat.error
yrError Age estimation.
massfloatphys.massMsunMass
e_massfloatphys.massMsunError Mass
log_Avfloatstat.error
phys.absorption
log_10(Av) optical extinction. See McMillan et al 2017, §2.1
elog_Avfloatstat.error
phys.absorption
Error of log_10(Av) optical extinction. . See McMillan et al 2017, §2.1
parallaxfloatpos.parallaxmasspectrophotometric Parallax (McMillan et al. 2017)
eparallaxfloatstat.error
pos.parallax
masError of spectrophotometric Parallax (McMillan et al. 2017)
dist_modfloatphot.mag.distModmagDistance Modulus from McMillan et al. 2017
edist_modfloatphot.mag.distModmagError of distance Modulus from McMillan et al. 2017
Teff_PJMdoublephys.temperature.effectiveKEffective temperature from reverse pipeline (McMillan et al 2017)
eTeff_PJMdoublephys.temperature.effectiveKError effective temperature from reverse pipeline (McMillan et al 2017)
logg_PJMdoublephys.gravitydexLog gravity from reverse pipeline (McMillan et al 2017)
elogg_PJMdoublephys.gravitydexLog gravity from reverse pipeline (McMillan et al 2017)
N_Gauss_fitintmeta.numberNumber of components required for multi-aussian distance modulus fit
Gauss_mean_1floatstat.fit.paramProperty of multi-Gaussian distance modulus fit, see McMillan et al. 2017, eq. 4
Gauss_sigma_1floatstat.fit.paramProperty of multi-Gaussian distance modulus fit, see McMillan et al. 2017, eq. 4
Gauss_frac_1floatstat.fit.paramProperty of multi-Gaussian distance modulus fit, see McMillan et al. 2017, eq. 4
Gauss_mean_2floatstat.fit.paramProperty of multi-Gaussian distance modulus fit, see McMillan et al. 2017, eq. 4
Gauss_sigma_2floatstat.fit.paramProperty of multi-Gaussian distance modulus fit, see McMillan et al. 2017, eq. 4
Gauss_frac_2floatstat.fit.paramProperty of multi-Gaussian distance modulus fit, see McMillan et al. 2017, eq. 4
Gauss_mean_3floatstat.fit.paramProperty of multi-Gaussian distance modulus fit, see McMillan et al. 2017, eq. 4
Gauss_sigma_3floatstat.fit.paramProperty of multi-Gaussian distance modulus fit, see McMillan et al. 2017, eq. 4
Gauss_frac_3floatstat.fit.paramProperty of multi-Gaussian distance modulus fit, see McMillan et al. 2017, eq. 4
FitQuality_Gaussfloatmeta.code.qualGiven by symbol F in eq. 5 of McMillan et al. 2017
Fit_Flag_Gaussintmeta.code.qualSee paragraph 2.1 (McMillan et al. 2017)
AV_Schlegeldoublephys.absorptionmagTotal Extinction in V-band from Schlegel et al. (1998)
logg_N_Kdoublephys.gravitydexLog gravity (Note 2, DR5)
elogg_Kdoublephys.gravitydexLog gravity (Note 2, DR5)
Teff_IRfloatphys.temperature.effectiveKEffective temperature from infrared flux method
eTeff_IRfloatstat.error
phys.temperature.effective
KError of effective temperature from infrared flux method
Met_N_Kdoublephys.abund.ZdexCalibrated metallicity [m/H]
eMet_Kdoublephys.abund.ZdexError of [m/H]
parallax_TGASdoublepos.parallaxmasParallax
parallax_error_TGASdoublestat.error
pos.parallax
masError of parallax
Jmag_2MASSfloatphot.mag
em.IR.J
magJ selected default magnitude from 2MASS
eJmag_2MASSfloatstat.error
phot.mag
em.IR.J
magerror 2MASS J magnitude
Hmag_2MASSfloatphot.mag
em.IR.H
magH selected default magnitude from 2MASS
eHmag_2MASSfloatstat.error
phot.mag
em.IR.H
magerror 2MASS H magnitude
Kmag_2MASSfloatphot.mag
em.IR.K
magK selected default magnitude from 2MASS
eKmag_2MASSfloatstat.error
phot.mag
em.IR.K
magerror 2MASS K magnitude
W1mag_ALLWISEfloatphot.mag
em.opt
magW1 magnitude from ALLWISE
eW1mag_ALLWISEfloatstat.error
phot.mag
em.opt
magError W1 magnitude from ALLWISE
W2mag_ALLWISEfloatphot.mag
em.opt
magW2 magnitude from ALLWISE
eW2mag_ALLWISEfloatstat.error
phot.mag
em.opt
magError W2 magnitude from ALLWISE
Mgfloatphys.abund.Zdex[Mg/H] abundance of Mg
Mg_Nsmallintmeta.numberNumber of used spectral lines in calc. of [Mg/H]
Alfloatphys.abund.Zdex[Al/H] abundance of Al
Al_Nsmallintmeta.numberNumber of used spectral lines in calc. of [Al/H]
Sifloatphys.abund.Zdex[Si/H] abundance of Si
Si_Nsmallintmeta.numberNumber of used spectral lines in calc. of [Si/H]
Tifloatphys.abund.Zdex[Ti/H] abundance of Ti
Ti_Nsmallintmeta.numberNumber of used spectral lines in calc. of [Ti/H]
Fefloatphys.abund.Zdex[Fe/H] abundance of Fe
Fe_Nsmallintmeta.numberNumber of used spectral lines in calc. of [Fe/H]
Nifloatphys.abund.Zdex[Ni/H] abundance of Ni
Ni_Nsmallintmeta.numberNumber of used spectral lines in calc. of [Ni/H]
c1charmeta.code1.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])
c2charmeta.code2.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])
c3charmeta.code3.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])
c4charmeta.code4.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])
c5charmeta.code5.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])
c6charmeta.code6.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])
c7charmeta.code7.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])
c8charmeta.code8.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])
c9charmeta.code9.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])
c10charmeta.code10.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])
c11charmeta.code11.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])
c12charmeta.code12.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])
c13charmeta.code13.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])
c14charmeta.code14.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])
c15charmeta.code15.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])
c16charmeta.code16.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])
c17charmeta.code17.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])
c18charmeta.code18.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] )
c19charmeta.code19.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])
c20charmeta.code20.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])
SNRdoublestat.snr(R+)Signal/Noise Ratio of Kordopatis Pipeline
Algo_Conv_Ktinyintmeta.code.qualQuality Flag for Stellar Parameter pipeline,[0..4]
flag_lowloggtinyintmeta.code.qual0 => logg >= 2.0, 1 => logg <2.0
flag_outliertinyintmeta.code.qual0 => not outlier, 1 => outlier (TGAS & RAVE-only differ by more than 4 sigma
flag_Ntinyintmeta.code.qual0 => spectrum flagged as normal by first 3 labels from Matijevič et al (2012, ApJS, 200, 14), 1 => spectrum flagged as normal
flag_poletinyintmeta.code.qual0 => good TGAS region, 1 => source lies in problematic TGAS region near ecliptic pole (165 < lambda <195, beta < 30), see McMillan et al. 2017
flag_duptinyintmeta.code.qual0 => only/best spectrum of start in RAVEDR5, 1 => spectrum of same star with higher SNR is in RAVEDR5
flag_anytinyintmeta.code.qual0 => all five flags above are 0, 1 => any of the above flags are 1