Table C.1
CARMENES M-dwarf sample of high S/N template spectra corrected for telluric absorption.
| # | Karmn | Name | GJ | a | δ | Spectral type | J [mag] | # VIS obs | S/N | # NIR obs | S/N |
|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | J00051+457 | BD+44 4548 | 2 | 00 05 10.89 | +45 47 11.6 | M1.0 | 6.70 | 53 | 833 | 44 | 756 |
| 2 | J00067-075 | GJ1002 | 1002 | 00 06 43.20 | −07 32 17.0 | M5.5 | 8.32 | 91 | 641 | 80 | 948 |
| 3 | J00162+198E | LP 404−062 | 1006B | 00 16 16.15 | +19 51 50.5 | M4.0 | 8.89 | 19 | 295 | 17 | 333 |
| 4 | J00183+440 | GX And | 15A | 00 18 22.88 | +44 01 22.6 | M1.0 | 4.85 | 222 | 2040 | 196 | 2230 |
| 5 | J00184+440 | GQ And | 15B | 00 18 25.82 | +44 01 38.1 | M3.5 | 6.79 | 195 | 1539 | 179 | 1972 |
| 6 | J00286-066 | GJ 1012 | 1012 | 00 28 39.46 | −06 39 49.2 | M4.0 | 8.04 | 50 | 714 | 43 | 803 |
| 7 | J00389+306 | Wolf 1056 | 26 | 00 38 59.04 | +30 36 58.4 | M2.5 | 7.45 | 61 | 911 | 55 | 944 |
| 8 | J00403+612 | 2MASS J00402129+6112490 | 00 40 21.29 | +61 12 49.1 | Ml.5 | 10.15 | 46 | 233 | 42 | 182 | |
| 9 | J00570+450 | G 172−030 | 00 57 02.69 | +45 05 09.8 | M3.0 | 8.10 | 20 | 432 | 17 | 495 | |
| 10 | J01013+613 | GJ47 | 47 | 01 01 20.05 | +61 21 56.7 | M2.0 | 7.27 | 10 | 307 | 9 | 251 |
| 11 | J01019+541 | G 218-020 | 3069 | 01 01 59.49 | +54 10 57.7 | M5.0 | 9.78 | 21 | 202 | 18 | 279 |
| 12 | J01025+716 | Ross 318 | 48 | 01 02 32.24 | +71 40 47.3 | M3.0 | 6.30 | 120 | 1183 | 103 | 1231 |
| 13 | J01026+623 | BD+61 195 | 49 | 01 02 38.87 | +62 20 42.2 | Ml.5 | 6.23 | 83 | 927 | 80 | 969 |
| 14 | J01033+623 | V388 Cas | 51 | 01 03 19.84 | +62 21 55.8 | M5.0 | 8.61 | 26 | 302 | 23 | 368 |
| 15 | J01048-181 | GJ 1028 | 1028 | 01 04 53.80 | -18 07 28.6 | M5.0 | 9.39 | 112 | 389 | 98 | 438 |
| 16 | J01066+192 | LSPM J0106+1913 | 01 06 36.98 | + 19 13 33.2 | M3.0 | 9.34 | 66 | 428 | 59 | 403 | |
| 17 | J01078+128 | G2−21 | 01 07 52.23 | + 12 52 51.8 | Ml.5 | 8.79 | 17 | 328 | 14 | 254 | |
| 18 | J01125−169 | YZCet | 54.1 | 01 12 30.64 | −16 59 56.4 | M4.5 | 7.26 | 113 | 974 | 101 | 1197 |
| 19 | J01339-176 | LP 768-113 | 01 33 58.00 | −17 38 23.8 | M4.0 | 8.84 | 29 | 342 | 27 | 440 | |
| 20 | J01352-072 | Barta 161 12 | 01 35 13.92 | −07 12 51.5 | M4.0 | 8.96 | 11 | 218 | 10 | 290 |
Notes. In the last four columns, we show the number of spectra we used to build the templates as well as the S/N per pixel in order 70 (~8600 Å) for the VIS and in order 52 (~10 500 Å) for the NIR. Equatorial coordinates, spectral types (class V), and J magnitudes were gathered from the CARMENES Cool dwarf Information and daTa Archive (Carmencita, see Alonso-Floriano et al. 2015, Caballero et al. 2016b, and references therein). The full table can be downloaded from the CDS.
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