Table 1.
SXTs with estimated average accretion rates and quiescent thermal luminosities.
| No. | Source | Remark (a) |
|---|---|---|
| 1 | 4U 2129+47 (V* V1727 Cyg) | In NGC 7078 |
| 2 | KS 1731−260 | CC, QP |
| 3 | 4U 1608−522 | |
| 4 | EXO 1745−248 (Ter 5 X-1) | In Terzan 5 |
| 5 | 1M 1716−315 (1H 1715-321) | |
| 6 | RX J1709.5−2639 | |
| (XTE J1709−267) | In NGC 6293 | |
| 7 | MXB 1659−29 (XB 1658−298) | CC, QP, E |
| 8 | 1RXS J173546.9−302859 | |
| (XB 1732−304) | In Terzan 1 | |
| 9 | 4U 1456−32 (Cen X-4) | |
| 10 | 1H 1905+00 (4U 1857+01) | |
| 11 | SAX J1806.8−2435 (2S 1803−245) | |
| 12 | 4U 1730−22 | |
| 13 | EXO 1747−214 | |
| 14 | XTE 2123−058 | |
| 15 | SAX J1810.8−2609 | |
| 16 | 4U 1908+005 (Aql X-1) | CC |
| 17 | SAX J1748.9−2021 (NGC 6440 X-1) | In NGC 6440 |
| 18 | CXOGlb J174852.7−202124 | UC |
| (NGC 6440 X-2) | in NGC 6440 | |
| 19 | XTE J0929−314 (V* BW Ant) | UC |
| 20 | SAX J1808.4−3658 (V* V4580 Sgr) | |
| 21 | XTE J1807−294 | UC |
| 22 | XTE J1751−305 | UC |
| 23 | XTE J1814−338 (V* V5511 Sgr) | |
| 24 | IGR J00291+5934 (V* V1037 Cas) | |
| 25 | HETE J1900.1−2455 | CC, QP |
| 26 | XTE J1701−462 | CC, QP |
| 27 | IGR J17480−2446 | CC |
| (Ter 5 X-2) | in Terzan 5 | |
| 28 | EXO 0748−676 (V* UY Vol) | CC, QP, E |
| 29 | 1RXS J180408.9−342058 | CC |
| 30 | Swift J174805.3−244637 | CC |
| (Ter 5 X-3) | in Terzan 5 | |
| 31 | SAX J1750.8−2900 | |
| 32 | Swift J1756.9−2508 | UC |
| 33 | Swift J1750.7−3117 | E |
| (GRS 1747−312) | in Terzan 6 | |
| 34 | IGR J18245−2452 | In Messier 28 |
| 35 | MAXI J0556−332 | CC, QP |
Notes.
The first column gives the sequential number for a quick reference; the second column lists the most common source identifiers in the literature; and the last column indicates a particular source type or association. UC – ultra-compact source (Van et al. 2019), E – eclipser, QP – quasi-persistent source, CC – crust cooling source (Wijnands et al. 2017).
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