Table B.1
List of the 40 newly observed stars.
N | Name | V | B-V | Teff | log(g) | Av | R | x0 | γ | c3 | Reference |
---|---|---|---|---|---|---|---|---|---|---|---|
(mag) | (mag) | (K) | (mag) | (μm−1) | (μm−1) | ||||||
Post-AGB | |||||||||||
3 | NGC 1535 | 12.11 | − 0.038* | 70 000 | 4.6 | 0.19 | Werner et al. (2003) | ||||
4 | HD 107969 | 13.2 | − 0.4 | 82 000 | 5.5 | 0.07 | Werner et al. (2003) | ||||
5 | LSS 1362 | 12.30 | − 0.22 | 100 000 | 5.3 | 0.56 | 3.67 | 4.62 | 1.21 | 6.03 | Werner et al. (2003) |
6 | PN A66-78 | 13.25 | − 0.21 | 110 000 | 5.5 | 0.57 | 3.24 | 4.70 | 1.07 | 2.88 | Werner et al. (2003) |
8 | NGC 7094 | 13.68 | − 0.050* | 110 000 | 5.7 | 0.41 | 2.98 | 4.70 | 1.35 | 6.21 | Werner et al. (2003) |
9 | PN K 1-16 | 14.96 | − 0.52 | 140 000 | 6.4 | 0.13 | Werner et al. (2003) | ||||
10 | NGC 6853 | 14.09 | − 0.34 | 110 000 | 6.7 | 0.08 | Werner et al. (2003) | ||||
11 | LSV+46 21 | 12.87 | − 0.37 | 83 000 | 6.7 | 0.16 | Werner et al. (2003) | ||||
13 | LSIII+52 24 | 12.51 | 0.72 | 24 000 | 3.0 | 2.07 | 3.08 | 4.89 | 2.85 | 40.64 | Sarkar et al. (2012) |
14 | LSIV-12 111 | 11.4 | − 0.1 | 20 500 | 2.35 | 0.88 | 2.98 | 4.63 | 1.16 | 4.14 | Ryans et al. (2003) |
16 | GLMP 334 | 12.3 | 0.8 | 7400 | 1.4 | 1.81 | 2.79 | 4.60 | 0.99 | 3.50 | Pereira et al. (2012) |
17 | NGC 3242 | 10.3 | 0.0 | 68 000 | 4.6 | 0.20 | 2.8 | 4.81 | 1.27 | 4.57 | Mendez et al. (1988) |
18 | NGC 1535 | 12.11 | − 0.038* | 58 000 | 4.3 | 0.21 | 2.83 | 4.73 | 1.13 | 3.65 | Mendez et al. (1988) |
19 | IC 2448 | 11.1 | 0.0 | 55 000 | 4.5 | 0.20 | Mendez et al. (1988) | ||||
21 | NGC 2392 | 10.52 | − 0.15 | 47 000 | 3.6 | 0.44 | 3.27 | 4.66 | 1.11 | 1.82 | Mendez et al. (1988) |
22 | Hen 2-182 | 11.72 | 0.31 | 36 000 | 3.4 | 0.86 | 3.75 | 4.76 | 2.12 | 20.4 | Mendez et al. (1988) |
23 | PN Tc 1 | 11.49 | − 0.19 | 33 000 | 3.2 | 0.62 | 3.06 | 4.67 | 1.03 | 3.34 | Mendez et al. (1988) |
Normal O Type | |||||||||||
25 | HD 93250 | 7.50 | 0.16 | 51 000 | 3.90 | 1.70 | 3.49 | 4.64 | 1.05 | 3.24 | Vacca et al. (1996) |
26 | HDE 303308 | 6.17 | 0.13 | 48 000 | 3.91 | 1.23 | 3.00 | 4.60 | 0.86 | 2.52 | Vacca et al. (1996) |
27 | HD 164794 | 5.97 | 0.0 | 47 000 | 3.90 | 1.02 | 3.28 | 4.58 | 0.94 | 3.26 | Vacca et al. (1996) |
28 | HD 46150 | 6.73 | 0.13 | 46 900 | 3.85 | 1.08 | 2.82 | 4.61 | 0.91 | 3.57 | Vacca et al. (1996) |
29 | HD 168075 | 8.77 | 0.55 | 49 000 | 3.95 | 2.28 | 3.15 | 4.62 | 0.99 | 3.23 | Vacca et al. (1996) |
30 | BD +60 513 | 9.39 | 0.49 | 40 000 | 3.70 | 2.17 | 2.85 | 4.58 | 0.89 | 3.32 | Vacca et al. (1996) |
31 | HD 217086 | 7.66 | 0.64 | 40 000 | 3.71 | 2.62 | 2.96 | 4.57 | 0.81 | 2.83 | Vacca et al. (1996) |
32 | HD 46966 | 6.87 | − 0.04 | 38 100 | 3.89 | 0.66 | 2.77 | 4.62 | 1.04 | 4.42 | Vacca et al. (1996) |
33 | NGC 6611 367 | 9.45 | 0.26 | 35 000 | 4.15 | 1.65 | 3.07 | 4.61 | 0.85 | 2.63 | Vacca et al. (1996) |
34 | HD 93521 | 7.03 | − 0.24 | 33 500 | 3.95 | 0.11 | Vacca et al. (1996) | ||||
35 | HD 228199 | 9.34 | 0.07 | 30 000 | 3.91 | 0.96 | 2.53 | 4.64 | 0.92 | 3.50 | Vacca et al. (1996) |
36 | HD 15570 | 8.11 | 0.69 | 49 000 | 3.51 | 2.85 | 2.87 | 4.62 | 0.72 | 2.30 | Vacca et al. (1996) |
37 | HD 192639 | 7.11 | 0.35 | 38 000 | 3.37 | 1.59 | 2.62 | 4.58 | 0.86 | 3.15 | Vacca et al. (1996) |
38 | HD 207198 | 5.94 | 0.31 | 34 000 | 3.31 | 1.44 | 2.63 | 4.65 | 1.08 | 3.96 | Vacca et al. (1996) |
39 | HD 210839 | 5.05 | 0.24 | 40 000 | 3.50 | 1.36 | 2.81 | 4.60 | 1.00 | 4.31 | Vacca et al. (1996) |
Horizontal Branch | |||||||||||
41 | GJ 894.3 | 11.50 | − 0.05 | 40 000 | 5.00 | 0.01 | Heber et al. (1984) | ||||
43 | PHL 382 | 11.4 | − 0.1 | 18 200 | 4.1 | 0.10 | Heber (1987) | ||||
47 | SB 707 | 11.9 | − 0.3 | 34 000 | 6.0 | 0.00 | Lamontagne et al. (1985) | ||||
50 | HD 205805 | 10.158 | − 0.241 | 25 000 | 5.0 | 0.01 | Altmann & de Boer (2000) | ||||
58 | DR And | 12.42 | 1.24 | 6200 | 2.3 | 0.00 | Pancino et al. (2015) | ||||
60 | EGB 5 | 14.2 | − 0.9 | 42 000 | 5.8 | 0.06 | Mendez et al. (1988) | ||||
64 | HD 269696 | 11.138 | − 0.297 | 40 000 | 5.5 | 0.03 | Lynas-Gray et al. (1984) | ||||
66 | RX Cet | 11.2 | 0.4 | 6186 | 2.0 | 0.00 | Pancino et al. (2015) | ||||
70 | RX J0122.9-7521 | 15.4 | − 0.4 | 180 000 | 7.5 | 0.54 | 4.54 | 4.53 | 1.20 | 2.02 | Werner & Herwig (2006) |
Notes. The columns are as follows: internal catalog number based on the 70 SNAP-mode candidate stars, name of the star, apparent magnitude through the V filter, color index, effective temperature, surface gravity, extinction in V , the ratio of total to selective extinction at V , bump position, bump width, and bump strength. The internal catalog number becomes the HST dataset number if you prepend the characters “ocy5,” so that, for example, star 33 is HST dataset ocy533. (*) PAGB stars missing B–V have, instead, J–K from the 2MASS point source catalog.
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