Table 3.
Targets used to build the masks employed to compute the CCFs of the low v sin i stars with their spectral types, rotational velocities, and magnitudes.
| Karmn | Name | Sp. | v sin i(a) | J(b) | VIS template |
VIS mask | NIR template |
NIR mask | ||
|---|---|---|---|---|---|---|---|---|---|---|
| type | [km s−1] | [mag] | # obs | S/N | # lines | # obs | S/N | # lines | ||
| J12123+544S | GJ 458A | M0.0 V | ≤2.0 | 6.88 | 110 | 1189 | 2019 | 105 | 1423 | 157 |
| J11033+359 | GJ 411 | M1.5 V | ≤2.0 | 4.20 | 310 | 1907 | 3762 | 300 | 2247 | 166 |
| J19169+051N | GJ 752A | M2.5 V | ≤2.0 | 5.58 | 129 | 1194 | 4332 | 125 | 1381 | 201 |
| J07274+052 | GJ 273 | M3.5 V | ≤2.0 | 5.71 | 733 | 1090 | 5334 | 721 | 1663 | 283 |
| J13229+244 | GJ 3779 | M4.0 V | ≤2.0 | 8.73 | 113 | 701 | 5423 | 110 | 1022 | 269 |
| J20260+585 | GJ 1253 | M5.0 V | ≤2.0 | 9.03 | 183 | 667 | 6136 | 182 | 991 | 443 |
| J10564+070 | GJ 406 | M6.0 V | 2.9 | 7.09 | 79 | 517 | 4382 | 76 | 1078 | 353 |
| J02530+168 | Teegarden’s star | M7.0 V | ≤2.0 | 8.39 | 245 | 732 | 5387 | 244 | 1528 | 389 |
Notes. We also show the number of observations used to build the templates, the S/N of a reference order (order 82 in the VIS and order 58 in the NIR), and the number of lines of the final mask in the VIS (from order 108 to order 68, 5623−9068 Å) and NIR channels (from order 63 to order 36, 9618−17 118 Å).
References.
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