Table 1.
Confirmed and candidate blue stars in the Leo P MUSE field.
LP# | MSB | α (J2000) | δ (J2000) | V | I | F475W | F814W | S/N | Comments |
---|---|---|---|---|---|---|---|---|---|
1 | 138 | 10 21 43.66 | +18 05 28.50 | 24.40 | 23.90 | 24.459 | 24.087 | 4 | Candidate |
2 | 207 | 10 21 43.71 | +18 05 21.69 | 24.79 | 24.64 | 24.737 | 24.819 | 5 | Candidate |
3 | 94 | 10 21 43.89 | +18 05 19.35 | 23.98 | 23.68 | 24.156 | 23.880 | 7 | Candidate |
4 | 16 | 10 21 43.92 | +18 05 56.59 | 22.50 | 22.29 | 22.521 | 22.561 | 19 | RV(Hβ) = 240 ± 19 km s−1 |
5 | 202 | 10 21 43.97 | +18 05 19.29 | 24.83 | 24.09 | 24.973 | 24.046 | 4 | Candidate |
6 | 40 | 10 21 44.01 | +18 05 23.81 | 23.45 | 23.08 | 23.707 | 23.348 | 8 | |
7 | 98 | 10 21 44.37 | +18 05 29.45 | 24.09 | 23.52 | 24.613 | 24.431 | 5 | Candidate |
8 | ... | 10 21 44.39 | +18 05 25.31 | ... | ... | 24.419 | 24.318 | 9 | |
9 | 92 | 10 21 44.47 | +18 05 25.62 | 23.95 | 23.66 | 24.111 | 23.961 | 6 | Candidate |
10 | ... | 10 21 44.55 | +18 05 20.00 | ... | ... | 23.958 | 24.013 | 9 | Candidate |
11 | ... | 10 21 44.63 | +18 05 16.14 | ... | ... | 23.834 | 23.908 | 4 | Candidate |
12 | ... | 10 21 44.69 | +18 05 21.07 | ... | ... | 24.363 | 24.488 | 7 | Candidate |
13 | ... | 10 21 44.69 | +18 05 23.47 | ... | ... | 24.090 | 24.155 | 9 | Candidate |
14 | 25 | 10 21 44.76 | +18 05 27.17 | 23.14 | 23.00 | 23.276 | 23.421 | 10 | Be/Ae? (Hα em.?) |
15 | ... | 10 21 44.79 | +18 05 25.15 | ... | ... | 24.251 | 24.540 | 7 | Candidate |
16 | 15 | 10 21 44.81 | +18 05 22.31 | ... | ... | 22.790 | 23.021 | 21 | |
17 | ... | 10 21 44.89 | +18 05 24.33 | ... | ... | 24.634 | 24.850 | 8 | |
18 | 12 | 10 21 44.90 | +18 05 22.38 | 22.16 | 22.02 | 22.255 | 22.304 | 28 | RV(Hβ) = 274 ± 19 km s−1 |
19 | 41 | 10 21 44.95 | +18 05 06.28 | 23.46 | 23.37 | 23.483 | 23.497 | 8 | |
20 | ... | 10 21 44.97 | +18 05 24.72 | ... | ... | 24.768 | 24.511 | 6 | Candidate |
21 | ... | 10 21 45.00 | +18 05 25.59 | ... | ... | 22.579 | 22.568 | 15 | RV(Hβ) = 260 ± 22 km s−1 |
22 | 24 | 10 21 45.01 | +18 05 13.21 | 23.15 | 22.87 | 23.369 | 23.308 | 11 | Be/Ae? (Hα & Hβ em.?) |
23 | ... | 10 21 45.03 | +18 05 24.80 | ... | ... | 22.473 | 22.585 | 12 | RV(Hβ) = 247 ± 20 km s−1 |
24 | ... | 10 21 45.03 | +18 05 25.02 | ... | ... | 23.066 | 23.052 | 3 | Candidate |
25 | ... | 10 21 45.08 | +18 05 16.35 | ... | ... | 24.290 | 24.684 | 15 | On SE edge of H II region |
26 | 2 | 10 21 45.10 | +18 05 16.62 | ... | ... | 21.464 | 21.837 | 52 | O-type star in H II region |
27 | 82 | 10 21 45.12 | +18 05 06.92 | 23.92 | 23.36 | 24.322 | 23.740 | 5 | Candidate |
28 | 22 | 10 21 45.13 | +18 05 13.76 | 23.01 | 23.16 | 22.999 | 23.349 | 13 | Candidate |
29 | 33 | 10 21 45.14 | +18 05 20.31 | 23.27 | 23.09 | 23.480 | 23.465 | 7 | |
30 | 63 | 10 21 45.21 | +18 05 09.09 | 23.73 | 23.41 | 24.435 | 24.488 | 8 | |
31 | 114 | 10 21 45.26 | +18 05 29.82 | 24.17 | 23.89 | 24.294 | 24.276 | 4 | Candidate |
32 | 106 | 10 21 45.27 | +18 05 07.84 | 24.11 | 23.90 | 24.238 | 24.080 | 5 | Candidate |
Notes.
Identifiers in the second column and V- and I-band photometry are from (MSB, McQuinn et al. 2013); F475W and F814W photometry is from the HST imaging from McQuinn et al. (2015). S/N estimates (per pixel) were obtained over the 5050–5400 Å part of the normalised spectra.
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