Table 1.
Basic stellar parameters of the sample taken from Simbad.
| HD | Name | Object type | SpT | Teff (K) | log g (dex) | Fe/H (dex) | Reference |
|---|---|---|---|---|---|---|---|
| 1835 | 9 Cet | BY* | G2.5 V |
 |
 |
 |
Boeche & Grebel (2016) |
| 10476 | 107 Psc | PM* | K1 V |
 |
 |
 |
Boeche & Grebel (2016) |
| 13421 | 64 Cet | PM* | G0 IV |
 |
 |
 |
Niedzielski et al. (2016) |
| 18256 | ρ Ari | SB* | F6 V |
 |
 |
 |
Balachandran (1990) |
| 20630 | κ1 Cet | BY* | G5 V |
 |
 |
 |
Boeche & Grebel (2016) |
| 25998 | 50 Per | RS* | F7 V |
 |
 |
 |
Chen et al. (2000) |
| 35296 | 111 Tau | BY* | F8 V |
 |
 |
 |
Prugniel et al. (2011) |
| 39587 | χ1 Ori | RS* | G0-V |
 |
 |
 |
Boeche & Grebel (2016) |
| 72905 | π1 UMa | BY* | G1.5 V |
 |
 |
 |
Boeche & Grebel (2016) |
| 75332 | – | PM* | F7 Vn |
 |
 |
 |
Chen et al. (2000) |
| 81809 | – | SB* | G2 V |
 |
 |
 |
Boeche & Grebel (2016) |
| 82443 | DX Leo | BY* | K0 V |
 |
 |
 |
Mishenina et al. (2013) |
| 82885 | 11 LMi | RS* | G8 IV-V |
 |
 |
 |
Boeche & Grebel (2016) |
| 103095 | – | PM* | G8 V |
 |
 |
 |
Boeche & Grebel (2016) |
| 115383 | η Vir | PM* | G0 Vs |
 |
 |
 |
Boeche & Grebel (2016) |
| 115404 | – | ** | K1 V |
 |
 |
 |
Boeche & Grebel (2016) |
| 120136 | τ Boo | ** | F6 IV |
 |
 |
 |
Boeche & Grebel (2016) |
| 124570 | 14 Boo | ** | F6 IV |
 |
 |
 |
Takeda (2007) |
| 129333 | EK Dra | BY* | G0 V |
 |
 |
 |
König et al. (2005) |
| 131156A | ξ Boo A | PM* | G8 V |
 |
 |
 |
Boeche & Grebel (2016) |
| 143761 | ρ CrB | PM* | G0+ Va |
 |
 |
 |
Boeche & Grebel (2016) |
| 149661 | 12 Oph | BY* | K2 V |
 |
 |
 |
Boeche & Grebel (2016) |
| 158614 | – | SB* | G9 IV-V |
 |
 |
 |
Boeche & Grebel (2016) |
| 161239 | 84 Her | PM* | G2 IIIb |
 |
 |
 |
Niedzielski et al. (2016) |
| 182572 | 31 Aql | PM* | G7 IV |
 |
 |
 |
Boeche & Grebel (2016) |
| 185144 | σ Dra | PM* | K0 V |
 |
 |
 |
Boeche & Grebel (2016) |
| 190007 | – | BY* | K4 V |
 |
 |
 |
Boeche & Grebel (2016) |
| 201091 | 61 Cyg A | BY* | K5 V |
 |
 |
 |
Boeche & Grebel (2016) |
| 201092 | 61 Cyg B | Fl* | K7 V |
 |
 |
 |
Boeche & Grebel (2016) |
| 206860 | HN Peg | BY* | G0 V |
 |
 |
 |
Ramírez et al. (2013) |
Notes. Spectral types have been adopted from Messina & Guinan (2002) and Lockwood et al. (2007). The object type reads as follows: BY* = Variable of BY Dra type, RS* = Variable of RS CVn type, PM* = High proper-motion star, SB* = Spectroscopic binary, ** = Double or multiple star, Fl* = Flare star.
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