Table 4.
Optical counterparts of eRASSU J050810.4–660653, RX J0501.6–7034, and eRASSt J044811.1–691318.
Source | V(a) | Q(a,b) | 2MASS | J | H | Ks | RA | Dec. | D(d) |
---|---|---|---|---|---|---|---|---|---|
(short) | (J2000) (c) | ||||||||
(mag) | (mag) | (mag) | (mag) | (mag) | (h m s) | (°′″) | (″) | ||
J0508 | 14.15 | −0.89 | 05080993−6606523 | 13.98 | 13.93 | 13.70 | 05 08 09.94 | −66 06 52.1 | 0.61 |
J0501 | 14.36 | −0.84 | 05012419−7033346 | 13.98 | 13.17 | 13.06 | 05 01 23.84 | −70 33 33.9 | 0.95 |
J0448 | 15.77 | −0.76 | – | – | – | – | 04 48 10.65 | −69 13 17.0 | 0.99 |
Notes.
Magnitudes and colours are taken from Zaritsky et al. (2004) or in the case of eRASSt J044811.1–691318 from Massey (2002).
Reddening-free parameter, defined as Q = U − B − 0.72(B − V). For the distribution of the Q parameter of BeXRBs in the SMC; see Haberl & Sturm (2016).
Position of the optical counterpart from Gaia EDR3 (see Gaia Collaboration 2021, 2016).
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