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Table 4.

Clump candidates.

Clump ID RA Dec Nbins F0.5 − 3 keV Area Significance
(1) (2) (3) (4) (5) (6) (7)
BC1 1:03:34.1026 −22:12:58.368 48 3.37 × 10−5 17419 21.1
BC2 1:03:12.3089 −22:12:49.189 13 1.58 × 10−5 8188 18.0
C3 1:03:19.7836 −21:33:26.717 3 1.73 × 10−6 824 7.62
C4 1:03:08.8609 −21:38:51.309 1 9.24 × 10−7 696 2.37
C5 1:03:13.4436 −21:40:53.937 3 3.33 × 10−6 1862 5.24
C6 1:03:46.7412 −21:46:45.169 1 3.48 × 10−7 184 3.09
C7 1:03:23.0879 −21:48:28.149 1 8.32 × 10−7 212 3.93
C8 1:03:58.0752 −21:52:57.118 6 4.38 × 10−6 4290 8.33
C9 1:03:33.8031 −21:53:59.633 7 4.38 × 10−6 1446 9.82
C10 1:01:34.3747 −21:39:44.730 2 1.14 × 10−6 308 8.06
C11 1:01:58.5747 −21:27:18.801 1 1.72 × 10−6 1180 2.39
C12 1:04:14.2142 −21:48:07.787 1 4.78 × 10−7 401 3.19
C13 1:02:11.6771 −22:00:34.794 1 3.53 × 10−6 2024 2.07
C14 1:02:06.3268 −22:00:47.524 1 1.22 × 10−6 664 2.18
C15 1:02:03.7572 −22:05:09.921 1 6.34 × 10−7 525 2.17
C16 1:01:47.1879 −22:02:33.340 1 8.83 × 10−7 738 2.16

Notes. Columns are as follows: (1) Clump ID. (2) and (3) central coordinates of each clump. (4) The number of neighboring outlier bins that were grouped. (5) Total flux of each clump candidate, in units of photon cm−2 s−1. (6) Area of the clump, in units of arcsec2. (7) Significance of the clump in σ.

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