Table C.1.
Comparison of the spectral type derived for low-mass stars with those listed in the literature.
| # | Spectral type from: |
|||||
|---|---|---|---|---|---|---|
| This work | Lépine et al. (2013) | CARMENCITA (a) | SpT vs. V–J | Other(s) | Refs. | |
| relation (b) | ||||||
| 2 | M3.5V | M4V | ... | M3.4 | M3.5+M3.6, M4V | 9, 11 |
| 3 | M2.5V | ... | M2.5V | M2.4 | M2.4V | 8 |
| 5 | M4V | M4V | M4V+M | M3.6 | M4.0+M4.5, M3.7V | 7, 8 |
| 6c2 | M1V | ... | ... | M0.4 | M2V | 6 |
| 9 | M1V | M1.5V | ... | M1.2 | ... | ... |
| 12 | M2.5V | ... | ... | M0.9 | ... | ... |
| 14 | M3.5V | ... | ... | M0.8 | ... | ... |
| 15 | M0.5V | ... | ... | M3.1 | ... | ... |
| 20 | ... | ... | ... | M2.4 | ... | ... |
| 21 | M3V | ... | ... | M3.6 | M2e | 5 |
| 23 | M3.5V | ... | ... | M1.9 | ... | ... |
| 24 | M1.5V | M2V | M1V | M2.7 | M3 | 2 |
| 26 | M0.5V | ... | ... | M2.5 | ... | ... |
| 29 | M0V | ... | ... | M1.0 | ... | ... |
| 30 | M4V | ... | ... | M3.7 | ... | ... |
| 34 | M1V | ... | ... | M1.8 | ... | ... |
| 35 | M0.5V | ... | ... | M1.3 | ... | ... |
| 38 | M0V | ... | ... | K7.85 | K5/M0 | 3 |
| 39 | M3.5V | ... | ... | M3.8 | ... | ... |
| 48 | ... | M4V | M3.5V | M4.1 | M4/5 | 10 |
| 54 | ... | ... | ... | M2.8 | M3/4 | 10 |
| 61 | ... | ... | ... | M1.0 | ... | ... |
| 62 | ... | M4V | ... | M4.1 | ... | ... |
| 69 | ... | ... | ... | M2.4 | ... | ... |
| 70 | M3V | M2.5V | ... | M1.7 | ... | ... |
| 73 | M1V | ... | ... | M1.4 | ... | ... |
| 80 | M1.5V | ... | ... | M1.9 | ... | ... |
| 81c1 | M1V | ... | ... | ... | ... | ... |
| 81c2 | M2.5V | ... | ... | ... | ... | ... |
| 85 | M2V | ... | ... | M1.2 | M2V | 11 |
| 88 | M4V | M4V | M3.5V | M3.6 | M4Ve | 4 |
| 107 | M0V | ... | ... | M0.5 | ... | ... |
| 111 | M1V | ... | ... | M1.4 | ... | ... |
| 113 | M0V | M0V | ... | M0.6 | ... | ... |
| 121 | M3.5V | ... | ... | M4.6 | ... | ... |
| 124 | K7V | ... | ... | M0.2 | ... | ... |
| 136 | K6V | ... | ... | M0.2 | ... | ... |
| 143 | M0V | ... | ... | M2.0 | ... | ... |
| 146 | M0.5V | ... | ... | M2.6 | ... | ... |
| 151 | M0V | M0.5V | M0V | M1.0 | M0V, M0.3V | 1, 8 |
| 154 | M0.5V | ... | ... | M1.9 | ... | ... |
| 161 | M1.5V | ... | ... | M2.6 | ... | ... |
| 189 | K7V | ... | ... | M1.1 | ... | ... |
| 191c1 | M0V | ... | ... | M1.2 | K7V | 6 |
| 191c2 | M2V | ... | ... | ... | M3V | 6 |
Notes.
CARMENCITA stands for “CARMENes Cool star Information and daTa Archive” and is a private database of the CARMENES consortium (http://carmenes.caha.es/).
We converted the V–J color index into spectral type by using Eq. (12) of Lépine et al. (2013).
References. 1 = Vyssotsky (1956); 2 = Lee (1984); 3 = Stephenson (1986); 4 = Fleming et al. (1988); 5 = Motch et al. (1998); 6 = Tachihara et al. (2005); 7 = Daemgen et al. (2007); 8 = Shkolnik et al. (2009); 9 = Shkolnik et al. (2010); 10 = Gigoyan & Mickaelian (2012); and 11 = Janson et al. (2012).
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