Table 2: continued.
1 16 17 18 19 20 21
No. $d_{\rm R}$ HRI PSPC [HS2000] Source ID Remarks
  [ $^{\prime\prime}$]          
01 - - - - RX J0051.7-7341 XRB?
02 22.8 - 547 28 SMC X-2 HMXB Be, P
03 4.5 058 241 31 RX J0054.9-7226 HMXB Be, P
04 - - - 32 XMMU J005605.2-722200 = 2E 0054.4-7237? HMXB?, P
05 5.6 - 234 - 2E 0055.6-7241, RX J0057.3-7225 AGN, z = 0.15
06            
06a - - - - XMMU J005735.7-721932 = [YIT2000] 19? new HMXB?
07 8.1 073 114 35 AX J0058-720, RX J0057.8-7202 HMXB?, P
08 7.3 074 136 36 RX J0057.8-7207 HMXB?, P
09 4.3 076 - 38 RX J0058.2-7231 HMXB Be
10 2.9          
10a 4.7 081 218 - RX J0059.3-7223 XRB?
11 6.6 088 123 - RX J0100.2-7204 XRB? AGN?
12 - - - - XMMU J010030.2-722035 new HMXB?
13 4.8          
13a 9.8 093 132 42 RX J0101.0-7206 HMXB Be
14 6.3 -        
14a 6.3 095 159 43 RX J0101.3-7211 HMXB Be, P
15 5.3          
15a 7.4 096 121 44 RX J0101.6-7204 HMXB?
16 4.6 101 143 49 AX J0103-722, SAX J0103.2-7209 HMXB Be, P
17 2.6 105 106 50 RX J0103.6-7201 HMXB?
18 6.9 - 120 55 RX J0105.9-7203 HMXB?
Notes to Col. 16: Distance to ROSAT source.
Notes to Cols. 17-19: Entry numbers in ROSAT HRI catalogue (Sasaki et al. 2000), ROSAT PSPC catalogue (Haberl et al. 2000), and Haberl & Sasaki (2000).
Notes to Col. 20: YIT2000: Yokogawa et al. (2000).
Notes to Col. 21: HMXB: High mass X-ray binary, HMXB?: HMXB candidate, XRB?: X-ray binary candidate, Be: Be system, P: pulsar.

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