Open Access

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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