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Table A.1.

Derived atmospheric parameters of the XSL stars.

Name Obs (a) UVB solution VIS solution Adopted parameters flag (b)
Teff logg [Fe/H] Teff logg [Fe/H] Teff err logg err [Fe/H] err
(K) (cm s−2) (Sun) (K) (cm s−2) (Sun) (K) (cm s−2) (Sun)
2MASS J17535707−2931427 247 4723 2.03 −0.04 4722 2.31 −0.02 4723 37 2.03 0.15 −0.04 0.05
2MASS J18024572−3001120 255 4495 1.57 1.00 3296 1.82 −0.08 3296 35 1.82 0.82 −0.28 2.27
2MASS J18024611−3004509 256 2700 5.71 1.00 3096 0.79 0.21 3096 67 0.69 0.30 0.01 0.25
2MASS J18025277−2954335 257 3328 1.44 0.39 3368 0.33 −0.25 3368 56 0.23 0.20 −0.45 0.20
2MASS J18032525−2959483 169 3270 0.50 −0.32 3270 56 0.40 0.22 −0.52 0.24
2MASS J18033716−2954227 152 4237 2.49 0.34 4297 2.56 0.52 4250 30 2.55 0.15 0.45 0.05
2MASS J18040638−3010497 153 3354 1.19 0.57 3384 0.39 −0.04 3384 56 0.29 0.20 −0.24 0.19
2MASS J18042244−3000534 154 2958 0.88 −0.09 3240 1.03 −0.08 3240 41 1.03 0.21 −0.28 0.20
... ... ... ... ... ... ... ... ... ... ... ... ... ...

Notes.

(a)

XSL observation identifier. Internal unique number for an observation; repeated observations of the same target have different numbers, so this number should not be used to identify a star.

(b)

Flag for stars that show large differences with their literature stellar parameters (if there are at least two literature measurements available), as discussed in Sect. 4.6. Carbon stars studied by Gonneau et al. (2016, 2017) have also been flagged. The flags should be combined with the quality flags for the spectra from the XSL DR2 paper (Gonneau et al., in prep).

This table is available in its entirety at the CDS.

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