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Table 1

Coordinates and atmospheric parameters for the program stars based in the analysis of the low-resolution spectra with FERRE.

Star g RA Dec T eff log g [Fe / H] [C / Fe] S/N a Survey
mag h ′′ ′′ K cm s-2

SDSS J015131+163944 18.9 01:51:31.2 +16:39:44.98 5917 3.9 –3.6 1.3 19 BOSS
SDSS J030444+391021 17.8 03:04:44.97 +39:10:21.17 5918 4.9 –3.7 0.3 29 SEGUE
SDSS J105519+232234 17.8 10:55:19.28 +23:22:34.03 6448 4.9 –4.2 –0.3 32 BOSS
SDSS J132917+542027 14.9 13:29:17.34 +54:20:27.52 5876 0.5 –4.0 47 LAMOST
SDSS J134157+513534 15.4 13:41:57.97 +51:35:34.08 6011 1.5 –4.9 35 LAMOST
SDSS J134338+484426 12.6 13:43:38.66 +48:44:26.48 5390 1.0 –3.7 0.7 56 SEGUE
SDSS J152202+305526 16.6 15:22:02.09 +30:55:26.29 5500 0.6 –4.1 37 SEGUE
SDSS J173329+332941 18.9 17:33:29.32 +33:29:41.94 6448 4.5 –4.2 0.7 21 SEGUE
SDSS J200513104503 17.0 20:05:13.48 –10:45:03.21 6488 4.4 –3.7 –0.7 45 SEGUE
SDSS J202109+601605 17.9 20:21:09.01 +60:16:05.33 5834 3.3 –3.4 0.4 20 SEGUE
SDSS J204524+150825 16.7 20:45:24.03 +15:08:25.46 5069 2.4 –3.6 0.0 39 SEGUE
SDSS J231027+231003 17.3 23:10:27.16 +23:10:03.43 6188 4.1 –4.0 33 SEGUE
SDSS J222505+164322 18.0 22:25:05.97 +16:43:22.52 5378 1.0 –3.7 0.9 24 BOSS

Notes.

(a)

Signal-no-noise ratio have been calculated as average of the SDSS or LAMOST entire spectrum.

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