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Table 7

X-ray sources in the SMC field with significant short-term variability.

SRC RA Dec Class log (Cst)a N b SRC RA Dec Class log (Cst)a N b
1 01 17 05.2 −73 26 36 HMXB <−40 316 817 851 01 10 57.6 −73 05 14 ⟨fg−star⟩ −13.06 290
2 01 18 38.0 −73 25 27 fg−star −39.36 13 873 852 01 16 33.5 −72 59 49 AGN −5.51 1008
7 01 19 39.4 −73 27 33 ⟨fg−star⟩ −3.63 171 884 01 00 13.9 −73 07 25 ⟨fg−star⟩ −17.02 2022
9 01 16 27.9 −73 14 47 ⟨AGN⟩ o? −3.08 153 885 01 00 37.2 −73 00 36 ⟨fg−star⟩ <−40 1067
37 01 14 55.6 −73 15 33 ⟨fg−star⟩ −2.58 280 888 01 00 39.2 −73 16 55 −9.01 211
51 01 01 20.7 −72 11 19 HMXB −3.73 1081 905 00 55 02.1 −73 21 15 ⟨fg−star⟩ −15.30 290
61 00 55 35.4 −72 29 07 HMXB −4.67 505 923 01 17 50.1 −73 30 09 −4.18 55
63 00 54 56.3 −72 26 47 HMXB −3.37 463 934 01 16 35.0 −73 37 43 ⟨AGN⟩ o? −2.97 10
66 00 56 18.9 −72 28 03 ⟨HMXB⟩ −2.70 214 937 01 13 53.2 −73 27 08 ⟨ClG⟩ −2.38 119
92 00 54 46.3 −72 25 23 HMXB −8.26 1160 948 01 16 21.7 −73 29 32 −13.49 33
112 00 47 23.3 −73 12 28 HMXB −31.48 7094 1032 00 59 14.3 −72 20 12 ⟨fg−star⟩ −4.87 21
113 00 51 52.2 −73 10 34 HMXB −6.92 10 189 1041 00 53 07.8 −74 39 06 fg−star <−40 241 087
137 00 52 15.1 −73 19 16 ⟨HMXB⟩ −4.97 387 1194 01 05 46.8 −72 02 34 ⟨AGN⟩ o? −8.93 63
146 00 48 59.2 −72 58 17 ⟨fg−star⟩ −13.08 214 1199 01 02 23.2 −72 11 35 ⟨fg−star⟩ −2.59 11
149 00 57 49.4 −72 02 36 HMXB <−40 6024 1399 00 55 18.3 −72 38 52 HMXB −5.35 1551
165 00 59 40.8 −72 19 05 −2.47 22 1462 00 52 03.0 −72 05 05 ⟨AGN⟩ o? −2.40 219
183 00 58 58.7 −72 01 12 ⟨fg−star⟩ −3.36 20 1481 00 42 07.8 −73 45 03 ⟨HMXB⟩ −6.64 315
184 01 01 52.3 −72 23 33 HMXB −6.16 999 1483 00 41 55.3 −73 34 16 ⟨AGN⟩ o? −2.35 131
187 01 03 14.0 −72 09 14 HMXB −2.63 1322 1500 00 42 21.2 −73 27 58 ⟨fg−star⟩ −8.80 29
197 01 05 09.9 −72 11 47 ⟨AGN⟩ ox −3.20 189 1525 00 44 18.5 −73 37 00 ⟨AGN⟩ o? −2.50 28
216 01 02 06.7 −71 41 16 HMXB −7.85 1948 1560 00 43 02.2 −72 52 34 ⟨AGN⟩ o? −4.48 428
227 01 03 37.6 −72 01 33 HMXB −9.15 7426 1617 01 02 08.0 −72 47 32 ⟨AGN⟩ o? −2.51 19
228 01 05 55.4 −72 03 49 HMXB −3.57 235 1700 00 50 05.6 −73 32 01 ⟨AGN⟩ o? −2.31 30
231 01 01 37.7 −71 54 15 ⟨fg−star⟩ −8.88 199 1702 00 49 13.5 −73 25 60 ⟨fg−star⟩ −2.51 21
239 01 05 50.3 −71 57 60 ⟨fg−star⟩ −2.74 65 1755 01 03 42.6 −71 57 58 −17.86 36
255 01 05 00.3 −72 11 48 ⟨fg−star⟩ −4.26 29 1802 00 52 05.7 −72 26 05 HMXB −2.32 2592
256 01 05 37.5 −71 57 19 −2.34 22 1998 00 50 12.1 −71 46 54 ⟨fg−star⟩ −4.35 28
287 01 01 55.9 −72 10 28 ⟨HMXB⟩ −2.95 28 2002 00 47 17.6 −71 55 20 ⟨AGN⟩ o? −2.54 42
335 00 54 55.9 −72 45 11 HMXB −3.58 3038 2041 01 03 16.5 −71 31 42 ⟨fg−star⟩ <−40 1014
352 00 53 24.2 −72 39 41 ⟨AGN⟩ o? −2.32 10 2381 00 42 38.8 −72 33 27 AGN r −17.31 606
392 00 52 58.5 −70 50 22 ⟨AGN⟩ o? −2.55 19 2454 00 43 47.7 −73 02 08 ⟨AGN⟩ o? −2.42 27
402 01 09 30.0 −72 52 49 ⟨AGN⟩ o? −2.94 580 2601 00 56 45.4 −72 59 32 −5.50 154
407 01 08 25.9 −72 54 31 fg−star −2.44 352 2651 00 54 50.8 −72 51 26 ⟨AGN⟩ o? −4.05 14
487 00 45 24.1 −73 29 07 ⟨fg−star⟩ −4.39 451 2735 01 09 35.2 −72 11 45 fg−star <−40 708
542 00 59 29.5 −71 58 09 ⟨AGN⟩ oi −2.66 31 2738 01 10 50.8 −72 10 25 AGN r −2.66 332
556 01 02 14.7 −72 49 17 ⟨AGN⟩ oi −2.90 23 2740 01 09 18.6 −72 12 38 ⟨fg−star⟩ −3.49 204
562 01 03 31.7 −73 01 44 ⟨HMXB⟩ −2.49 19 2845 01 13 02.3 −72 41 42 ⟨fg−star⟩ −9.22 524
615 00 49 30.6 −73 31 09 HMXB −2.83 223 2846 01 11 54.6 −72 45 57 ⟨fg−star⟩ −11.28 304
636 00 48 46.6 −73 30 00 ⟨AGN⟩ o? −2.62 16 3059 01 13 04.2 −73 14 35 ⟨fg−star⟩ −9.03 103
654 00 53 23.9 −72 27 15 HMXB −3.16 2149 3115 01 06 33.0 −73 15 43 HMXB −11.24 811
668 00 54 38.5 −72 22 09 ⟨AGN⟩ o? −2.52 51 3167 01 02 28.0 −73 16 57 ⟨AGN⟩ o? −3.35 27
674 00 59 28.9 −72 37 04 HMXB −14.16 6464 3186 00 59 37.0 −73 25 41 ⟨AGN⟩ o? −2.31 127
730 00 49 22.8 −72 10 55 −2.64 81 3190 00 58 35.7 −73 14 48 ⟨fg−star⟩ −2.64 79
760 00 42 45.8 −73 10 14 ⟨fg−star⟩ −2.79 173 3267 00 50 34.6 −73 30 30 ⟨AGN⟩ o? −6.26 214
812 01 00 09.6 −72 57 49 ⟨AGN⟩ o? −15.07 1087

Notes.

(a)

Probability Cst that the source is constant during the observation. Minimum of all detections of the source is given.

(b)

Number of source counts of the detections with the given value of Cst.

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