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Table 1.

Sky regions used in the MST search for photon clusters.

Region Solid angle Photon number
Λm
Λcut
Nps
Ns
Nw
sr N S N S N S N S N S N S
|b|> 78° 0.1373 5083 3154 95 187 57 112 46 48 33 41 37 44

64° < |b|< 81° A 0.2824 11729 6299 87 142 52 85 95 99 69 65 79 74
64° < |b|< 81° B 0.2855 10034 5875 100 150 60 90 93 99 68 57 77 71

49° < |b|< 66° A 0.5045 18939 14109 98 121 59 73 176 202 111 110 128 129
49° < |b|< 66° B 0.5101 16820 13423 107 126 64 75 176 191 104 122 123 138

34° < |b|< 51° A 0.6923 27127 24953 101 110 61 66 332 333 143 126 171 154
34° < |b|< 51° B 0.6999 23800 23396 113 112 68 67 402 333 150 141 169 164

18° < |b|< 36° C 0.1995 14277 12031 81 87 48 52 219 191 23 26 26 28
18° < |b|< 36° D 0.7931 31554 28206 97 105 58 63 388 389 122 107 134 121
18° < |b|< 36° E 0.7444 25816 30296 113 104 68 63 392 396 121 109 131 123
18° < |b|< 36° F 0.1606 11325 8536 79 91 47 54 134 107 30 19 34 24

Notes. There is an overlap at each side of the regions. The total number of photons, the solid angle of the region for a single hemisphere, and the mean angular separation lengths for the north and south Galactic regions are given; the clearly evident N–S asymmetry is mainly due to the different exposures. In the last three columns we report the number of clusters found in each region with the primary selection and after the application of the secondary standard and weak selections, 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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