VizieR

CfA VizieR . ADAC VizieR . Cambridge (UK) VizieR . IUCAA VizieR . INASAN VizieR .

VizieR

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I/354/starhorse2021 StarHorse2, Gaia EDR3 photo-astrometric distances (Anders+, 2022)
Starhorse catalog 2021 (original column names in green) (362392321 rows)
  -c=288.2371662797 +15.7491890437, eq=ICRS, rs=2
Post annotation about this record
ColumnValue  Explain   (UCD)
_r0.000 arcsec Distance from center (288.2371662797+15.7491890437)[ICRS], at Epoch=J2016.0 (pos.angDistance)
_RAJ200019 12 56.919907126 "h:m:s" Right ascension (FK5, Equinox=J2000.0) at Epoch=J2016. (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services) (pos.eq.ra)
_DEJ2000+15 44 57.08055732 "d:m:s" Declination (FK5, Equinox=J2000.0) at Epoch=J2016. (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services) (pos.eq.dec)
_RAB195019 10 40.995949822 "h:m:s" Right ascension (FK4, Equinox=B1950.0) at Epoch=J2016. (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services) (pos.eq.ra)
_DEB1950+15 39 48.20690341 "d:m:s" Declination (FK4, Equinox=B1950.0) at Epoch=J2016. (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services) (pos.eq.dec)
_Glon049.369168020670 deg Galactic longitude at Epoch=J2016. (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services) (pos.galactic.lon)
_Glat+02.492427107204 deg Galactic latitude at Epoch=J2016. (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services) (pos.galactic.lat)

source_id4512794813113096320  (i) Gaia EDR3 unique source identifier (source_id) (meta.id;meta.main)
ra288.2371662797 deg (i) Barycentric right ascension of the source (ICRS) at Ep=2016.0 (ra) (Note 1)   (pos.eq.ra;meta.main)
dec+15.7491890437 deg (i) Barycentric declination of the source (ICRS) at Ep=2016.0 (dec) (Note 1)   (pos.eq.dec;meta.main)
mass16 0.949484 Msun StarHorse stellar mass 16th percentile (phys.mass)
mass50 1.086616 Msun StarHorse stellar mass 50th percentile (phys.mass)
mass84 1.149478 Msun StarHorse stellar mass 84th percentile (phys.mass)
teff16 5697.71 K StarHorse effective temperature 16th percentile (phys.temperature.effective)
teff50 6130.79 K StarHorse effective temperature 50th percentile (phys.temperature.effective)
teff84 6368.68 K StarHorse effective temperature 84th percentile (phys.temperature.effective)
logg16 4.175088 [cm/s2] StarHorse surface gravity 16th percentile (phys.gravity)
logg50 4.375350 [cm/s2] StarHorse surface gravity 50th percentile (phys.gravity)
logg84 4.461339 [cm/s2] StarHorse surface gravity 84th percentile (phys.gravity)
met16-0.440637 [-] StarHorse metallicity 16th percentile (phys.abund.Z)
met50-0.126707 [-] StarHorse metallicity 50th percentile (phys.abund.Z)
met84 0.234785 [-] StarHorse metallicity 84th percentile (phys.abund.Z)
dist05 1.511148 kpc StarHorse distance 5th percentile (pos.distance)
dist16 1.828544 kpc StarHorse distance 16th percentile (pos.distance)
dist50 2.218340 kpc StarHorse distance 50th percentile (pos.distance)
dist84 2.723566 kpc StarHorse distance 84th percentile (pos.distance)
dist95 3.270788 kpc StarHorse distance 95th percentile (pos.distance)
av05 2.000861 mag StarHorse line-of-sight extinction at λ=5420A 5th percentile (av05) (phys.absorption.gal)
av16 2.318882 mag StarHorse line-of-sight extinction at λ=5420A 16th percentile (av16) (phys.absorption.gal)
av50 2.618614 mag StarHorse line-of-sight extinction at λ=5420A 50th percentile (av50) (phys.absorption.gal)
av84 2.856413 mag StarHorse line-of-sight extinction at λ=5420A 84th percentile (av84) (phys.absorption.gal)
av95 2.906397 mag StarHorse line-of-sight extinction at λ=5420A 95th percentile (av95) (phys.absorption.gal)
fidelity 0.988281  Gaia EDR3 astrometric fidelity flag (Rybizki et al., 2021, MNRAS, in prep.) (meta.code)
xgal -6.756822 kpc StarHorse Galactocentric Cartesian X co-ordinate derived from dist50 and assuming R0=8.2kpc (xgal) (pos.cartesian.x;pos.galactocentric)
ygal 1.681952 kpc StarHorse Galactocentric Cartesian Y co-ordinate derived from dist50 and assuming R0=8.2kpc (ygal) (pos.cartesian.y;pos.galactocentric)
zgal 0.096470 kpc StarHorse Galactocentric Cartesian Z co-ordinate derived from dist50 and assuming R0=8.2kpc (zgal) (src.redshift;pos.galactocentric;pos.cartesian)
rgal 6.963017 kpc StarHorse Galactocentric planar distance derived from XGal and YGal (rgal) (pos.distance;pos.galactocentric)
sh_photoflagGBPRPgrizy/JH  StarHorse photometry input flag (sh_photoflag) (Note 2)   (meta.code.error)
sh_outflag 0  StarHorse output flag (sh_outflag) (Note 3)   (meta.code.error)
bp_rp_excess_corr 0.0205101970   Gaia EDR3 photometric BP/RP flux excess factor (corrected following Riello et al., 2021A&A...649A...3R) (bp_rp_excess_corr) (phot.flux;arith.ratio)
ag50 2.112100 mag StarHorse line-of-sight extinction in the G band derived from AV50 and teff50 (ag50) (phys.absorption)
abp50 2.670250 mag StarHorse line-of-sight extinction in the GBP band 50th percentile derived from AV50 and teff50 (abp50) (phys.absorption)
arp50 1.563161 mag StarHorse line-of-sight extinction in the GRP band 50th percentile derived from AV50 and teff50 (arp50) (phys.absorption)
mg0 4.113883 mag StarHorse absolute magnitude derived from photgmean_mag (recalibrated) dist50 and AG50 (mg0) (phys.magAbs)
bprp0 0.721224 mag StarHorse dereddened colour (GBP-GRP)0 derived from photbpmean_mag, photrpmean_mag ABP50 and ARP50 (bprp0) (phot.mag.reddFree)
  
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