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Table 3
Absorbed SSS candidates with possible early type star counterpart in the SMC.
| X-ray | MCPS | MA93 | |||||||||||
| RA | Dec | Δr | H R 1 | H R 2 | ML | d | U | B | V | I | d | cat. No | Comment |
| (J2000) | (J2000) | () | () | (mag) | (mag) | (mag) | (mag) | () | [MA93] | ||||
|
|
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| 01 17 40.44 | –73 30 50.7 | 1.3 | 0.6 ± 0.2 | –0.3 ± 0.2 | 11.8 | 1.3 | 13.3 | 14.1 | 14.2 | 14.1 | 0.4 | 1845 | HMXB |
| 01 05 16.05 | –72 00 25.0 | 2.1 | 0.9 ± 0.2 | –1.0 ± 0.1 | 10.6 | 5.2 | 14.9 | 15.8 | 16.0 | 16.2 | – | – | – |
| 00 59 54.57 | –72 15 30.5 | 1.8 | 1.0 ± 0.2 | –0.7 ± 0.2 | 12.3 | 4.4 | 15.8 | 16.8 | 16.9 | 17.0 | – | – | – |
| 00 49 13.54 | –73 25 60.0 | 1.8 | 0.3 ± 0.2 | –0.7 ± 0.2 | 15.5 | 0.8 | 14.6 | 15.4 | 15.4 | 15.1 | – | – | – |
| 01 01 05.01 | –72 04 43.5 | 3.3 | 0.3 ± 0.2 | –0.7 ± 0.2 | 23.7 | 5.5 | 15.3 | 16.2 | 16.4 | 16.6 | – | – | Gal. star? |
| 00 53 55.61 | –72 26 44.4 | 2.1 | 0.7 ± 0.3 | –0.5 ± 0.2 | 10.0 | 1.3 | 13.6 | 14.6 | 14.7 | 14.6 | – | – | HMXB |
| 00 51 52.50 | –72 31 47.8 | 1.6 | 0.5 ± 0.2 | –0.5 ± 0.2 | 10.8 | 3.1 | 13.7 | 14.8 | 14.4 | 14.4 | 3.4 | 506 | Gal. star? |
| 00 55 07.25 | –72 08 25.7 | 1.7 | –0.1 ± 0.3 | –0.6 ± 0.3 | 8.6 | 3.9 | 16.0 | 16.8 | 16.9 | 16.9 | – | – | HMXB? |
| 00 55 08.45 | –71 58 26.7 | 1.4 | –0.2 ± 0.2 | –0.9 ± 0.4 | 14.0 | 4.6 | 14.2 | 15.2 | 15.4 | 15.6 | – | – | – |
| 00 54 14.97 | –72 14 43.1 | 3.4 | 1.0 ± 0.5 | –1.0 ± 0.5 | 11.5 | 5.3 | 15.8 | 16.5 | 16.6 | 16.8 | 12.0 | 744 | – |
Notes. Δr: 1σ X-ray position uncertainty, including the systematic error. HR: X-ray hardness ratios. ML: detection likelihood. d: Angular distance to the counterpart from MCPS (Zaritsky et al. 2002) and MA93 (Meyssonnier & Azzopardi 1993).
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