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Table 2

Positions (J2000) and errors for detected sources.

# Name RA Dec Error Offset
(h m s) (°   ′   ′′) (′′) (′′)

Firm Swift/XRT detections
2 AX J1504.6–5824 15 04 30.92 –58 24 09.6 4.1 55.3
5 AX J1538.3–5541 15 38 13.68 –55 42 13.1 1.9 62.2
7 AX J1620.1–5002 16 20 06.76 –50 01 58.0 2.8 47.2
8 AX J1651.0–4403 16 51 11.43 –44 02 37.0 2.3 79.8
12 AX J1719.3–3703 17 19 20.88 –37 01 51.6 4.4 72.9
14 AX J1725.8–3533 17 25 49.31 –35 33 40.1 4.1 15.7
16 AX J1738.4–2902† 17 38 26.18 –29 01 49.6 2.2 3.0
18 AX J1742.6–3022 17 42 41.13 –30 22 36.8 2.8 75.9
19 AX J1742.6–2901 17 42 41.93 –29 02 09.7 3.4 5.6
22 AX J1754.2–2754† 17 54 14.47 –27 54 36.1 2.2 48.7
29 AX J1846.0–0231 18 45 56.81 –02 31 59.3 4.4 60.9

Tentative Swift/XRT detections
11 AX J1717.2–3718 17 17 24.01 –37 17 18.3 3.2 105
13 AX J1720.8–3710 17 20 51.64 –37 10 33.9 3.9 23.7
17 AX J1739.5–2730 17 39 35.86 –27 29 36.8 4.2 40.2
30 AX J1846.1–0239 18 46 03.75 –02 39 16.7 4.1 106
32 AX J1856.7+0220 18 56 43.82 +02 19 20.15 4.1 57.4

Notes. The quoted XRT positional uncertainties refer to a 90% confidence level. The offset from the ASCA position is listed in the last column. The two sources that are marked by a dagger have more accurate Chandra localisations that were recently published and are consistent with our Swift positions: AX J1754.2–2754 (Bassa et al. 2008) and AX J1738.4–2902 (Evans et al. 2010).

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