Table D.1
Gaia DR3 & VLT/FLAMES results for stars that are members of the Sextans dSph.
GaiaDR3Id Flamesfield Notes |
Gaia-RA SpecName |
Gaia-DEC N-Spec |
Gaia-G SN |
Gaia-BP Vel |
Gaia-RP vel-err |
plx vel-var |
plx-err FeH |
pmra feh-err |
pmra-err feh-var |
pmdec Pmem |
pmdec-err |
---|---|---|---|---|---|---|---|---|---|---|---|
3828546221455694464 | 152.3519 | -2.86573 | 19.257 | 19.667 | 18.717 | 0.269 | 0.287 | -0.239 | 0.352 | -0.234 | 0.444 |
Sextans-c18 | DM25 | 1 | 22.1 | 215.56 | 1.28 | 0.0 | -2.84 | 0.254 | 0.0 | 0.919 | |
3829021485356307712 | 152.86228 | -2.09496 | 17.356 | 17.985 | 16.619 | 0.186 | 0.096 | -0.335 | 0.099 | 0.041 | 0.103 |
Sextans-c9 W23 206.49 Aoki09 S15-19-3.22 |
DM57 | 1 | 64.3 | 206.55 | 0.34 | 0.0 | -2.93 | 0.065 | 0.0 | 1.0 | |
3829103325958201344 | 153.34061 | -1.79572 | 19.556 | 20.112 | 18.944 | -0.204 | 0.421 | -0.726 | 0.426 | 0.481 | 0.52 |
Sextans-cl Theler20 S11-141 |
DM850 | 1 | 13.1 | 211.95 | 1.77 | 0.0 | -2.36 | 0.321 | 0 | 1.0 | |
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We have included here all the Gaia DR3 likely members in this table even those without FLAMES spectra.
The columns are: GaiaDR3Id, Gaia DR3 Id number; Gaia-RA, right ascension (deg); Gaia-DEC, declination (deg); Gaia-G, Gaia DR3 G magnitude; Gaia-BP, Gaia DR3 GBP magnitude; Gaia-RP, Gaia DR3 GRP magnitude; plx, Gaia DR3 parallax; plx-err, Gaia DR3 error on the parallax; pmra, Gaia DR3 proper motion in RA direction; pmra-err, Gaia DR3 error on RA proper motion; pmdec, Gaia DR3 proper motion in DEC direction; pmdec-err, Gaia DR3 error on DEC proper motion; Flamesfield, name of the VLT/FLAMES pointing; SpecName, name of object in VLT/FLAMES pointing; N-Spec, number of individual VLT/FLAMES spectra combined; SN, the signal-to-noise of the single (for N-Spec=1) or combined VLT/FLAMES spectra; Vel, the υlos for this star measured from VLT/FLAMES spectra, averaged if N-spec> 1; vel-err, error on the υlos VLT/FLAMES measurement; vel-var, the variance of the VLT/FLAMES υlos if N-spec> 1; FeH, the [Fe/H]for the star determined from the CaT measurement from VLT/FLAMES spectra, averaged if N-spec> 1; feh-err, the error on the VLT/FLAMES [Fe/H]determination; feh-var, the variance of the VLT/FLAMES [Fe/H]if N-spec> 1; Pmem, probability of membership from B22 analysis; Notes refer to previous measurements of these stars: Walker et al. (2023) (W23) with the radial velocity, Theler et al. 2020; Shetrone et al. 2001; Aoki et al. 2009
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