Table 2
Sources.
| Name | obsid(s) | Distance | Coordinates | |
|---|---|---|---|---|
| kpc | l (deg) | b (deg) | ||
| GX 5-1 | 19449, 20119 | 9.2 (1) | 5.08 | −1.02 |
| GX 13+1 | 11814, 11815, 11816, 11817 | 7 ± 1(2) | 13.52 | +0.11 |
| GX 340+00 | 1921, 18085, 19450, 20099 | 11 ± 0.3(3) | 339.59 | −0.08 |
| GX 17+2 | 11088 | 12.6 (4) | 16.43 | +1.28 |
| 4U 1705-44 | 5500, 18086, 19451, 20082 | 7.6 ± 0.3(5) | 343.32 | −2.34 |
| 4U 1630-47 | 13714, 13715, 13716, 13717 | 10(6) | 336.91 | +0.25 |
| 4U 1728-34 | 2748 | 5.2 ± 0.5(7) | 354.30 | −0.15 |
| 4U 1702-429 | 11045 | 7 (8) | 343.89 | −1.32 |
| GRS 1758-258 | 2429, 2750 | 8.5 (9) | 4.51 | −1.36 |
Notes. Table with Chandra observations used in this paper, indicated by the obsids. All observations were done in TE mode. Coordinateswere taken from the SIMBAD database (Wenger et al. 2000).
References. Distances are taken from (1) Christian & Swank (1997), (2) Bandyopadhyay et al. (1999), (3) Christian & Swank (1997), (4) Lin et al. (2012), (5) Galloway et al. (2008), (6) Parmar et al. (1986); Augusteijn et al. (2001), (7)Galloway et al. (2008), (8)Oosterbroek et al. (1991), and (9)Keck et al. (2001).
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