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Table 2.

Sky regions used in the MST search for photon clusters.

Region Solid angle Photon number Λcut Nps Nss
sr N S N S N S N S
|b| > 79° 0.1154 4639 3162 7ʹ̣4 13ʹ̣3 58 127 20 28
64° < |b| < 81° A 0.2824 10521 6428 6ʹ̣8 10ʹ̣1 102 138 45 42
64° < |b| < 81° B 0.2955 9498 6014 7ʹ̣5 10ʹ̣5 105 154 42 44
49° < |b| < 66° A 0.5045 17267 14297 7ʹ̣4 8ʹ̣7 197 278 71 75
49° < |b| < 66° B 0.5101 16361 12570 7ʹ̣9 9ʹ̣4 228 266 65 81
34° < |b| < 51° A 0.6923 24822 24121 7ʹ̣6 8ʹ̣0 425 512 110 93
34° < |b| < 51° B 0.6999 23126 21469 8ʹ̣2 8ʹ̣4 564 435 107 86
19° < |b| < 36° C 0.1876 11769 10209 6ʹ̣1 6ʹ̣5 298 252 17 20
19° < |b| < 36° D 0.6544 25942 24282 7ʹ̣4 7ʹ̣8 466 510 94 89
19° < |b| < 36° E 0.7002 22555 25512 8ʹ̣4 7ʹ̣8 494 539 96 78
19° < |b| < 36° F 0.1510 9368 7060 5ʹ̣9 6ʹ̣8 208 147 24 15

Note. There is an overlap on each side of the regions. The total number of photons and the resulting separation lengths for the north and south Galactic regions are given; the well evident N-S asymmetry is mainly because of the different exposures. In the last two columns the number of clusters found in each region are reported with the primary selection and after the application of the secondary and superselection, as described in the text. The Galactic longitude intervals are A: 0° < l < 182°; B: 178° < l < 362°; C: 0° < l < 41°; D: 39° < l < 182°; E: 178° < l < 331°; and F: 329° < l < 362°.

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