Table 2
Properties of the spectral template stars observed with PPak.
| HD | SpT | log g | [Fe/H] | Ref. | Obs. Date | S/N | λ/Δλ | HD | SpT | log g | [Fe/H] | Ref. | Obs. Date | S/N | λ/Δλ |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
|
|
|||||||||||||||
| 123299 | A0 III | 3.30 | −0.56 | a | 2008-02-04 | 945 | 7293 | 63352 | K0 III | 2.20 | −0.31 | a | 2004-11-19 | 632 | 7676 |
| 6695 | A3 V | 4.30 | − | g | 2004-11-19 | 1091 | 7712 | 74442 | K0 III | 2.51 | −0.06 | a | 2005-11-02 | 527 | 7857 |
| 159561 | A5 III | 3.96 | +0.01 | g | 2008-02-04 | 1076 | 6905 | 85503 | K0 III | 2.33 | +0.23 | a | 2005-11-06 | 1145 | 7647 |
| 13267 | B5 Ia | 2.44 | − | a | 2004-11-19 | 760 | 7729 | 102224 | K0 III | 2.02 | −0.46 | a | 2006-10-14 | 472 | 6589 |
| 27295 | B9 IV | 3.93 | −0.74 | a | 2004-11-19 | 1129 | 7792 | 145328 | K0 III | 3.25 | −0.20 | b | 2005-05-02 | 618 | 8180 |
| 57118 | F0 Ia | 1.7 | − | g | 2004-11-19 | 612 | 7947 | 203344 | K0 III-IV | 2.62 | −0.24 | b | 2004-11-13 | 441 | 8322 |
| 29375 | F0 V | 4.17 | +0.13 | g | 2004-11-19 | 743 | 7920 | 7010 | K0 IV | 3.3 | − | g | 2004-11-19 | 296 | 7988 |
| 115604 | F3 III | 3.4 | +0.18 | e | 2004-11-19 | 1257 | 7891 | 16160 | K1 III | 1.88 | −0.25 | a | 2004-11-19 | 1388 | 7352 |
| 31236 | F3 IV | 4.21 | +0.13 | g | 2004-11-19 | 579 | 7825 | 23841 | K1 III | 1.30 | −0.95 | a | 2004-11-19 | 620 | 7766 |
| 43318 | F6 V | 3.93 | −0.15 | a | 2004-11-19 | 687 | 7791 | 162555 | K1 III | 2.72 | −0.21 | b | 2007-01-15 | 1083 | 8180 |
| 136202 | F8 III-IV | 3.85 | −0.08 | a | 2008-02-04 | 1112 | 6601 | 176411 | K1 III | 2.91 | +0.00 | b | 2005-05-02 | 927 | 8200 |
| 22879 | F9 V | 4.29 | −0.83 | a | 2004-11-19 | 632 | 7632 | 205512 | K1 III | 2.57 | +0.03 | a | 2006-10-15 | 732 | 7476 |
| 101501 | G0-8 Vv | 4.60 | −0.13 | a | 2004-11-19 | 1473 | 7745 | 51440 | K2 III | 2.28 | −0.35 | a | 2004-11-19 | 993 | 7957 |
| 18391 | G0 Ia | 0.00 | −0.28 | a | 2004-11-19 | 441 | 7975 | 72184 | K2 III | 2.61 | +0.12 | a | 2005-11-06 | 871 | 7937 |
| 6903 | G0 III | 2.9 | − | g | 2004-11-19 | 851 | 7612 | 162211 | K2 III | 2.45 | +0.05 | a | 2006-08-24 | 829 | 7661 |
| 30455 | G2 V | 4.45 | −0.36 | g | 2004-11-19 | 612 | 7848 | 163588 | K2 III | 2.61 | −0.09 | b | 2007-01-15 | 839 | 7842 |
| 6474 | G4 Ia | 1.50 | +0.25 | a | 2004-11-19 | 301 | 7807 | 83618 | K3 III | 1.74 | −0.08 | a | 2005-11-06 | 1046 | 7400 |
| 82210 | G4 III-IV | 3.19 | −0.28 | a | 2008-02-04 | 937 | 7155 | 94247 | K3 III | 2.24 | −0.27 | b | 2004-11-19 | 1302 | 7881 |
| 157910 | G5 III | 1.83 | −0.32 | a | 2007-01-15 | 1306 | 8081 | 97907 | K3 III | 2.07 | −0.10 | a | 2004-11-13 | 870 | 7572 |
| 107950 | G6 III | 2.61 | −0.16 | b | 2008-02-04 | 861 | 7124 | 102328 | K3 III | 2.09 | +0.35 | a | 2005-05-03 | 1129 | 7647 |
| 175535 | G7 IIIa | 2.55 | −0.09 | a | 2007-01-12 | 1173 | 8296 | 127665 | K3 III | 2.22 | −0.17 | b | 2007-01-15 | 1114 | 8223 |
| 184492 | G8-9 III | 2.59 | −0.10 | b | 2005-05-02 | 487 | 8179 | 143107 | K3 III | 2.34 | −0.32 | b | 2005-05-02 | 1419 | 8216 |
| 6833 | G8 III | 1.25 | −0.99 | a | 2004-11-19 | 602 | 7911 | 184406 | K3 III | 2.41 | +0.01 | a | 2005-05-02 | 836 | 8295 |
| 38656 | G8 III | 2.52 | −0.22 | a | 2006-10-14 | 727 | 7405 | 48433 | K3 V | 4.55 | −0.07 | d | 2004-11-19 | 710 | 7261 |
| 57264 | G8 III | 2.72 | −0.33 | a | 2008-02-04 | 836 | 7549 | 149161 | K4 III | 1.39 | −0.17 | a | 2005-05-02 | 770 | 8211 |
| 65714 | G8 III | 1.50 | +0.27 | a | 2004-11-19 | 975 | 7644 | 49161 | K4 III | 1.69 | +0.08 | a | 2004-11-19 | 1148 | 7364 |
| 103736 | G8 III | 2.3 | − | g | 2004-11-16 | 756 | 7660 | 148513 | K4 IIIp | 1.67 | +0.11 | a | 2005-05-02 | 635 | 8352 |
| 141680 | G8 III | 3.02 | −0.28 | b | 2005-05-02 | 789 | 8106 | 61603 | K5 III | 1.50 | +0.24 | a | 2004-11-19 | 875 | 7523 |
| 133640 | G8 IIIv? | − | − | g | 2007-01-14 | 661 | 7665 | 136028 | K5 III | 1.90 | +0.19 | g | 2005-05-02 | 384 | 8154 |
| 73593 | G8 IV | 2.25 | −0.12 | a | 2004-11-15 | 956 | 7733 | 146051 | M0.5 III | 1.40 | +0.32 | a | 2008-02-04 | 1023 | 6475 |
| 82885 | G8 IV-V | 4.61 | +0.00 | a | 2005-11-06 | 488 | 7711 | 137471 | M1 III | 1.10 | +0.07 | a | 2008-01-31 | 853 | 7642 |
| 41636 | G9 III | 2.50 | −0.20 | a | 2004-11-19 | 804 | 7903 | 167006 | M3 III | 0.70 | +0.00 | a | 2008-02-04 | 648 | 7106 |
| 104985 | G9 III | 2.52 | −0.26 | c | 2006-10-13 | 567 | 7153 | 123657 | M4 III | 0.85 | +0.00 | a | 2008-02-04 | 739 | 7164 |
| 180711 | G9 III | 2.67 | −0.12 | a | 2007-01-13 | 1235 | 8519 | 148783 | M6 III | 0.20 | −0.01 | f | 2008-02-04 | 839 | 6940 |
| 19476 | K0 III | 3.08 | +0.04 | b | 2006-10-13 | 940 | 7358 | ||||||||
Notes. (1) HD number; (2) spectral type; (3) surface gravitation; (4) metallicity; (5) reference; (6) date of observation; (7) signal-to-noise ratio (S/N); (8) effective instrumental spectral resolution (λ/Δλ). The template star used for the stellar-kinematic analysis in this paper (HD 162555) has been highlighted. The S/N and λ/Δλ are for the combined spectrum (Sect. 6.8.2). The spectral type, surface gravity and metallicity have been taken from the following references: (a) Cenarro et al. (2007); (b) McWilliam (1990); (c) Luck & Heiter (2007); (d) Soubiran et al. (2008); (e) Massarotti et al. (2008); (f) Ramírez et al. (2000); (g) N. Cardiel (priv. comm.).
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