Table 2: X-ray position (equatorial and Galactic) of the X-ray counterparts to the 17 sources studied with Swift/XRT.
Name RA Dec Error l b
(IGR) (J2000) (J2000) ( $^{\prime\prime}$) ($^\circ$) ($^\circ$)
J03184-0014$^\dagger$ 03$^{\rm h}$18$^{\rm m}$17.6$^{\rm s}$ -00$^\circ$17$^\prime $48.1 $^{\prime\prime}$ 5.7 181.8112 -45.7082
J03532-6829 03$^{\rm h}$52$^{\rm m}$57.4s -68$^\circ$31$^\prime $18.0 $^{\prime\prime}$ 3.5 282.8102 -40.7968
J05319-6601$^\dagger$ 05$^{\rm h}$31$^{\rm m}$52.6$^{\rm s}$ -65$^\circ$59$^\prime $40.2 $^{\prime\prime}$ 4.7 275.9037 -32.6650
J05346-5759 05$^{\rm h}$34$^{\rm m}$50.5$^{\rm s}$ -58$^\circ$01$^\prime $39.3 $^{\prime\prime}$ 3.5 266.4230 -32.7788
J09025-6814$^\dagger$ 09$^{\rm h}$02$^{\rm m}$39.4 -68$^\circ$13$^\prime $38.7 $^{\prime\prime}$ 4.8 284.1738 -14.1567
J10101-5654$^\star$ 10$^{\rm h}$10$^{\rm m}$11.9$^{\rm s}$ -56$^\circ$55$^\prime $31.6 $^{\prime\prime}$ 4.3 282.2567 -0.6719
J13000+2529$^\dagger$ 12$^{\rm h}$59$^{\rm m}$55.0$^{\rm s}$ +25$^\circ$28$^\prime $08.8 $^{\prime\prime}$ 6.9 352.2816 +87.4774
J13020-6359 13$^{\rm h}$01$^{\rm m}$59.2$^{\rm s}$ -63$^\circ$58$^\prime $06.0 $^{\prime\prime}$ 3.5 304.0891 -1.1202
J15161-3827$^\ddagger$ #1 15$^{\rm h}$15$^{\rm m}$59.3$^{\rm s}$ -38$^\circ$25$^\prime $48.3 $^{\prime\prime}$ 4.3 331.6935 +16.2381
#2 15$^{\rm h}$16$^{\rm m}$ 29.6$^{\rm s}$ -38$^\circ$26$^\prime $56.5 $^{\prime\prime}$ 4.6 331.7689 +16.1681
#3$^\dagger$ 15$^{\rm h}$16$^{\rm m}$12.7$^{\rm s}$ -38$^\circ$31$^\prime $02.4 $^{\prime\prime}$ 4.7 331.6819 +16.1411
#4$^\dagger$ 15$^{\rm h}$15$^{\rm m}$45.8$^{\rm s}$ -38$^\circ$27$^\prime $36.2 $^{\prime\prime}$ 4.7 331.6380 +16.2370
J15479-4529 15$^{\rm h}$48$^{\rm m}$14.7$^{\rm s}$ -45$^\circ$28$^\prime $40.4 $^{\prime\prime}$ 3.5 332.4403 +7.0228
J16287-5021$^\diamond$ 16$^{\rm h}$28$^{\rm m}$27.2$^{\rm s}$ -50$^\circ$22$^\prime $38.3 $^{\prime\prime}$ 4.4 334.1093 -1.1261
J17353-3539 17$^{\rm h}$35$^{\rm m}$23.5$^{\rm s}$ -35$^\circ$40$^\prime $13.8 $^{\prime\prime}$ 3.5 353.1445 -1.7401
J17476-2253 17$^{\rm h}$47$^{\rm m}$30.0$^{\rm s}$ -22$^\circ$52$^\prime $43.2 $^{\prime\prime}$ 4.8 5.3999 +2.7813
J18214-1318$^\star$ 18$^{\rm h}$21$^{\rm m}$19.7$^{\rm s}$ -13$^\circ$18$^\prime $38.2 $^{\prime\prime}$ 3.5 17.6813 +0.4856
J19267+1325$^\diamond$ 19$^{\rm h}$26$^{\rm m}$27.0$^{\rm s}$ +13$^\circ$22$^\prime $03.4 $^{\prime\prime}$ 3.7 48.8032 -1.5059
J20286+2544$^\ddagger$ #1 20$^{\rm h}$28$^{\rm m}$34.9$^{\rm s}$ +25$^\circ$43$^\prime $59.7 $^{\prime\prime}$ 3.9 67.0045 -7.5713
#2 20$^{\rm h}$28$^{\rm m}$28.7$^{\rm s}$ +25$^\circ$43$^\prime $22.5 $^{\prime\prime}$ 4.4 66.9825 -7.5582
J23206+6431 23$^{\rm h}$20$^{\rm m}$36.8$^{\rm s}$ +64$^\circ$30$^\prime $42.8 $^{\prime\prime}$ 3.8 113.3539 +3.3424
$^\dagger$ Source is very faint, just a very slight excess (very few photons) within IBIS error; $^\star$ consistent with the Chandra position published by Tomsick et al. (2008a); $^\ddagger$ several sources within IBIS error; $^\diamond$ consistent with the Chandra position published by Tomsick et al. (2008b).

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