Table E.5
Sample of hot star candidates.
| Id | RA | Dec | H | KS | location | EWCO | EWBry | FK ID | |
|---|---|---|---|---|---|---|---|---|---|
| F2_26655209-28824980_Ks10.63 | 266.55209 | -28.824980 | 12.23 | 10.63 | GC | -0.841 | 2.828 | vis | |
| F2_26655266-28819681_Ks11.80 | 266.55267 | -28.819681 | 13.29 | 11.80 | GC | -1.978 | 0.044 | vis | |
| F2_26655383-28816727_Ks8.90 | 266.55383 | -28.816727 | 10.97 | 8.90 | GC | -0.446 | 4.020 | vis | |
| F2_26655600-28816496_Ks9.86 | 266.55600 | -28.816496 | 11.60 | 9.86 | GC | -0.436 | -1.757 | vis | d |
| F2_26634747-29121044_Ks12.26 | 266.34747 | -29.121044 | 12.90 | 12.26 | fg | 4.126 | 0.237 | CO | |
| F2_26636584-29096720_Ks12.81 | 266.36584 | -29.096720 | 14.58 | 12.81 | GC | 1.818 | 0.742 | CO | |
| F2_26637106-29089252_Ks12.33 | 266.37106 | -29.089252 | 13.01 | 12.33 | fg | -0.302 | 0.940 | CO | |
| F2_26639999-29005692_Ks13.06 | 266.39999 | -29.005692 | 14.17 | 13.06 | GC | 4.264 | -1.509 | CO | |
| F2_26640643-28988766_Ks11.85 | 266.40643 | -28.988766 | 13.22 | 11.85 | GC | 4.153 | -0.751 | CO | |
| F2_26641107-28999369_Ks11.50 | 266.41107 | -28.999369 | 13.38 | 11.50 | GC | 4.211 | 1.761 | CO | |
| F2_26641314-29011974_Ks13.88 | 266.41315 | -29.011974 | 15.60 | 13.88 | GC | 4.732 | -7.683 | CO | |
| F2_26641345-29012257_Ks13.11 | 266.41345 | -29.012257 | 14.89 | 13.11 | GC | 3.428 | -3.423 | CO | |
| F2_26641806-29007921_Ks13.00 | 266.41806 | -29.007921 | 14.65 | 13.00 | GC | 4.555 | -28.845 | CO | 1387 b |
| F2_26641840-29005163_Ks13.10 | 266.41840 | -29.005163 | 15.09 | 13.10 | GC | 4.556 | -21.124 | CO | 1374 b |
| F2_26642648-29003094_Ks11.18 | 266.42648 | -29.003094 | 13.57 | 11.18 | GC | 4.442 | -1.398 | CO | |
| F2_26643866-28966084_Ks12.46 | 266.43866 | -28.966084 | 13.87 | 12.46 | GC | 4.485 | 0.693 | CO | |
| F2_26647446-28927660_Ks12.43 | 266.47446 | -28.927660 | 13.57 | 12.43 | GC | 3.023 | -1.049 | CO | |
| F2_26652917-28857695_Ks12.95 | 266.52917 | -28.857695 | 14.98 | 12.95 | GC | 4.597 | -1.108 | CO |
Notes. We list the name, coordinates RA and Dec, and observed H and Ks photometry. Our classification as GC star, foreground (fg) star, background (bg) star or unknown is based on the H - KS colour. The classification as hot stars was done via visual inspection of the spectra. Some of these stars have values of |EWCO|>5 Å due to bad pixels. We also list stars with spectra where weak CO absorption is visible, but only low(|EWCO|<5 Å.). We matched the list with the KMOS observations of Feldmeier-Krause et al. (2015, 2017a, 2020); Feldmeier-Krause (2022) and note the corresponding Id in the last column. (a) Early-type star in Feldmeier-Krause et al. (2015) (b)Late-type star in Feldmeier-Krause et al. (2017a) (c)Early-type star in Feldmeier-Krause (2022) (d)qF 381 in Clark et al. (2018b) (e)F2_26653436-28831776_Ks99.00 and F2_26653452-28831758_Ks10.13 may be the same star (f)Isolated massive star candidate in Clark et al. (2021)
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