Table 2: continued.
1 9 10 11 12 13 14 15
No. HR1 HR2 HR3 P $d_{\rm O}$ OGLE name [MA93]
        [s] [ $^{\prime\prime}$]    
01 +0.15 $\pm$ 0.20 +0.09 $\pm$ 0.18 -1.00 $\pm$ 0.26 - - - -
02 - - - too weak - - -
03 +0.41 $\pm$ 0.12 -0.03 $\pm$ 0.11 -0.30 $\pm$ 0.17 59.00 $\pm$ 0.02 1.2 00545617-7226476 810
04 +1.00 $\pm$ 0.23 -0.15 $\pm$ 0.17 -0.13 $\pm$ 0.25 140.1 $\pm$ 0.3* - - 904
05 +0.49 $\pm$ 0.05 -0.29 $\pm$ 0.05 -0.36 $\pm$ 0.08 - 1.8 00571981-7225337 -
06 +0.45 $\pm$ 0.11 +0.04 $\pm$ 0.09 -0.41 $\pm$ 0.11   1.9    
06a +0.80 $\pm$ 0.31 +0.10 $\pm$ 0.26 -0.54 $\pm$ 0.43 - 3.5 00573601-7219339 1020
07 +0.19 $\pm$ 0.09 +0.03 $\pm$ 0.08 -0.14 $\pm$ 0.10 281.1 $\pm$ 0.2 - - 1036
08 +0.48 $\pm$ 0.07 +0.25 $\pm$ 0.05 -0.06 $\pm$ 0.06 152.34 $\pm$ 0.05* - - 1038
09 +1.00 $\pm$ 0.33 +0.44 $\pm$ 0.21 +0.51 $\pm$ 0.13 - 4.5 00581258-7230485 -
10 +0.49 $\pm$ 0.07 -0.15 $\pm$ 0.07 -0.21 $\pm$ 0.10   1.2    
10a +0.27 $\pm$ 0.09 -0.05 $\pm$ 0.09 +0.12 $\pm$ 0.09 - 1.4 00592103-7223171 -
11 +0.18 $\pm$ 0.14 -0.19 $\pm$ 0.14 -0.46 $\pm$ 0.21 - - - -
12 +1.00 $\pm$ 0.13 -0.37 $\pm$ 0.29 +0.01 $\pm$ 0.52 - - - 1208
13 +0.37 $\pm$ 0.29 -0.30 $\pm$ 0.25 +0.06 $\pm$ 0.41        
13a -0.25 $\pm$ 0.36 -0.21 $\pm$ 0.48 +0.40 $\pm$ 0.41 - - - 1240
14 +0.14 $\pm$ 0.08 +0.21 $\pm$ 0.07 +0.06 $\pm$ 0.07 452.2 $\pm$ 0.5 2.6    
14a +0.26 $\pm$ 0.12 +0.06 $\pm$ 0.12 -0.10 $\pm$ 0.15 too weak 2.2 01012064-7211187 1257
15 +0.17 $\pm$ 0.10 -0.23 $\pm$ 0.10 -0.20 $\pm$ 0.16        
15a +0.17 $\pm$ 0.13 -0.36 $\pm$ 0.12 -0.26 $\pm$ 0.30 - - - 1277
16 +0.16 $\pm$ 0.07 +0.11 $\pm$ 0.06 +0.00 $\pm$ 0.06 341.7 $\pm$ 0.4 - - 1367
17 +0.28 $\pm$ 0.03 +0.18 $\pm$ 0.02 +0.07 $\pm$ 0.02 - - - 1393
18 -0.19 $\pm$ 0.18 +0.12 $\pm$ 0.18 +0.22 $\pm$ 0.16 - - - 1557
Notes to Cols. 9-11: Hardness ratios as defined in Eq. (1).
Notes to Col. 12: Pulse periods from timing analysis. * New X-ray binary pulsar!
Notes to Col. 13: Distance to OGLE object.
Notes to Col. 15: Entry numbers in Meyssonnier & Azzopardi (1993).

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