Table 4
Reddened magnitudes and colours of the 4 candidate counterparts to 2XMM J174016.0−290337.
| Star | J | H | K | J−H | J−K | H−K | Spectral Type | Distance |
| (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (kpc) | ||
|
|
||||||||
| 1 | 16.38 ± 0.12 | 15.07 ± 0.12 | 14.50 ± 0.12 | 1.30 ± 0.17 | 1.88 ± 0.17 | 0.57 ± 0.17 | – | – |
| 2 | 15.71 ± 0.06 | 15.01 ± 0.07 | 14.70 ± 0.08 | 0.70 ± 0.09 | 1.02 ± 0.10 | 0.31 ± 0.11 | M 5/6 V | 0.5 |
| 3 | 16.62 ± 0.08 | 15.21 ± 0.07 | 14.48 ± 0.07 | 1.41 ± 0.11 | 2.15 ± 0.11 | 0.73 ± 0.10 | – | – |
| 4 | 16.93 ± 0.09 | 15.70 ± 0.09 | 14.98 ± 0.08 | 1.22 ± 0.13 | 1.95 ± 0.12 | 0.72 ± 0.12 | – | – |
Notes. The colours of source 2 correspond to a foreground M 5/6 V star whose magnitudes indicate a distance of ~520 pc. The colours and magnitudes of the remaining 3 sources are inconsistent with any type of stellar source indicating they are heavily reddened, most likely in the Galactic Bulge (see Fig. 10).
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