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Table 9

Variable sources with flux variability greater than five, ordered by variability.

Source Fvar Svar Fmax‡ Efmax‡ Class+ Comment†
523 692.64 63.33 106.61 1.68 XRB
1032 660.61 54.21 33.89 0.62  ⟨ GlC ⟩  1(t, 92.2), 11, 16, 27(831.10)
57 644.03 96.796 147.76 1.52 XRB
1131 558.48 80.18 38.93 0.48  ⟨ XRB ⟩  1(t, 954.2), 2(t, 2163), 19, 20(t), 22, 26, 27(624.05)
944 236.47 44.74 24.24 0.54 XRB 1(t, 370.5), 14(t, BH-XRN), 20(t), 21(v,t), 26, 27(353.67)
705 185.02 39.85 32.52 0.81  ⟨ XRB ⟩  3(t), 27(178.79)
1007 161.84 42.33 44.30 1.04  ⟨ XRB ⟩  1, 12, 13, 26, 27(12.96)
1195 144.47 36.95 28.51 0.76  ⟨ SSS ⟩  2(t, 694), 14(v,t), 20(t), 26, 27(82.68)
1152 123.95 55.31 31.86 0.56  ⟨ XRB ⟩  1(t, 96.3), 2(t, 107), 9, 11(v), 12, 13(v), 19, 21(v,t), 26,
27(131.73)
788 117.83 20.99 12.27 0.58  ⟨ XRB ⟩  1(t, 20.8), 2(t, 93), 11, 14(t), 20(t), 26, 27(97.89)
1136 87.84 25.00 9.79 0.39  ⟨ XRB ⟩  1(t, 46.1), 2(t, 155), 19, 20(t), 23, 26, 27(97.65)
934 84.94 28.35 21.26 0.90  ⟨ SSS ⟩ 
949 80.16 25.55 17.75 0.68  ⟨ XRB ⟩  2(t, 13), 20, 25, 26
1194 75.22 39.69 12.79 0.31  ⟨ SSS ⟩  1, 2(t, 96), 9, 12, 13(v), 14(v), 19(v), 21(v), 26, 27(85.93)
1416 72.25 21.00 10.51 0.49  ⟨ SSS ⟩  26, 28
1084 59.11 8.70 6.64 0.75  ⟨ XRB ⟩  1(t, 79.0), 2(t, 260), 14(t), 18, 20(t), 21(v,t), 26, 27(57.41)
985 51.66 80.00 80.46 0.97 XRB 3(t), 5(t, LMXB), 9, 21(v), 27(76.27)
1017 49.85 20.73 9.64 0.45  ⟨ XRB ⟩  1(t, 99.5), 2(t, 158), 21(v,t), 26, 27(38.07)
990 48.90 61.77 82.16 1.28 XRB 1(t, 468.8), 2(t, 285), 14(v,t, BH-XRT), 18(t), 21(v,t), 26, 27(201.71)
1059 48.10 23.64 9.16 0.37  ⟨ XRB ⟩  1(t, 64.6), 27(39.69)
698 41.20 18.73 9.33 1.37  ⟨ XRB ⟩  13, 23, 26, 27(44.67)
884 32.88 9.59 2.84 0.61  ⟨ XRB ⟩  1, 27(24.95)
1153 31.06 17.96 4.22 0.22 XRB 1(t), 3(t), 6(t, LMXB), 27(30.50)
1000 26.86 20.17 5.75 0.48 1(t), 19, 21, 23, 26, 27(34.47)
1024 25.66 78.46 144.02 1.89  ⟨ XRB ⟩  1, 9, 11, 12, 13, 19, 21(v), 26, 27(34.02)
1177 24.00 19.31 4.59 0.22 XRB 3(t), 27(27.06)
939 22.48 10.13 2.20 0.20  ⟨ XRB ⟩  1(t, 65.2), 27(28.02)
960 21.56 9.497 5.51 0.55  ⟨ fg Star ⟩  1, 12, 13, 19, 21, 23, 26, 27(21.97)
1180 16.48 17.16 7.53 0.40  ⟨ XRB ⟩  1, 12, 19, 21(v), 26, 27(13.01)
378 16.21 9.39 6.83 0.98  ⟨ XRB ⟩  25, 26
714 14.89 13.77 10.35 0.68  ⟨ fg Star ⟩ 
748 14.45 13.86 3.62 0.23  ⟨ SSS ⟩  25, 26, 27(14.18)
92 14.23 5.73 1.86 0.30  ⟨ SSS ⟩ 
814 13.66 7.98 4.94 0.56  ⟨ XRB ⟩  1, 21(v), 25, 26, 27(15.76)
1006 11.30 14.34 1.44 0.08  ⟨ SSS ⟩  2(t, 51), 19, 23, 26, 27(10.70)
542 10.90 3.26 2.50 0.69  ⟨ XRB ⟩ 
1016 10.46 20.66 6.37 0.26  ⟨ XRB ⟩  1, 11 ,12, 19, 21, 26, 27(11.69)
1144 10.23 10.53 1.54 0.12  ⟨ SSS ⟩  2(t, 38), 26, 27(10.05)
1034 10.11 28.93 9.81 0.28  ⟨ XRB ⟩  1, 19, 21, 23, 27(10.24)
1099 9.95 4.50 5.12 1.01  ⟨ hard ⟩  25, 26
904 9.16 8.65 8.55 0.84  ⟨ hard ⟩  12, 26
872 9.13 17.16 7.31 0.38  ⟨ GlC ⟩  1, 7, 19 , 21(v), 26, 27(7.48)
1422 9.06 2.99 1.87 0.55  ⟨ hard ⟩ 
1183 7.66 11.93 8.43 0.57  ⟨ hard ⟩  12, 13, 26
422 7.23 9.65 2.10 0.16  ⟨ hard ⟩  13
823 7.16 28.29 20.25 1.30  ⟨ GlC ⟩  1, 4, 11, 14(v), 15, 19, 21(v), 26, 27(6.45)
1250 6.94 2.80 0.89 0.27  ⟨ SSS ⟩ 
398 6.79 2.93 1.79 0.52  ⟨ hard ⟩  13, 26
1266 6.67 7.54 2.37 0.24 GlC 4, 26, 27(8.27)
975 6.58 7.98 1.76 0.35 GlC 1, 4, 13, 15, 19, 20, 21(v), 26
522 6.47 6.62 2.21 0.26  ⟨ hard ⟩ 
805 6.22 3.66 0.96 0.21  ⟨ hard ⟩ 
916 6.21 3.73 2.00 0.44  ⟨ hard ⟩ 
862 6.17 5.33 1.38 0.20 GlC 1, 4, 15, 21, 26, 27(5.35)
1124 6.04 12.93 5.73 0.23  ⟨ GlC ⟩  1, 19, 20, 21(v), 26
430 5.98 4.95 1.01 0.16  ⟨ hard ⟩ 
1825 5.57 6.11 2.97 0.39 fg Star 13, 26
1494 5.55 4.06 0.95 0.18  ⟨ hard ⟩  26
624 5.54 7.58 1.49 0.13  ⟨ fg Star ⟩ 
1167 5.44 7.69 3.22 0.57  ⟨ hard ⟩  1, 19, 20, 21(v), 26
1450 5.44 6.51 2.24 0.24  ⟨ hard ⟩ 
66 5.39 3.80 2.31 0.49  ⟨ hard ⟩ 
1655 5.34 4.72 1.50 0.24  ⟨ hard ⟩ 
964 5.30 6.36 1.09 0.12  ⟨ hard ⟩ 
226 5.28 3.29 0.56 0.13  ⟨ hard ⟩ 
244 5.27 9.08 3.33 0.28  ⟨ hard ⟩  13, 25, 26
1361 5.21 3.12 1.36 0.34  ⟨ hard ⟩  27
933 5.19 4.99 8.73 1.30 GlC 4, 11, 12, 25, 26
1366 5.13 3.02 1.05 0.27  ⟨ hard ⟩ 

Notes. 

(‡)

Maximum flux and error in units of 1  ×  10-14 erg cm-2 s-1or maximum luminosity and error in units of 7.3  ×  1035 erg s-1;

(+)

class according to Table 6.

References. 

(†)

1: Voss & Gilfanov (2007), 2: Williams et al. (2006b), 3: Trudolyubov et al. (2006), 4: Trudolyubov & Priedhorsky (2004), 5: Williams et al. (2006a), 6: Williams et al. (2005b), 7: Pietsch & Haberl (2005), 8: Kong et al. (2003), 9: Trinchieri & Fabbiano (1991), 10: Collura et al. (1990), 11: Primini et al. (1993), 12: Supper et al. (1997), 13: Supper et al. (2001), 14: Osborne et al. (2001), 15: Di Stefano et al. (2002), 16: Fan et al. (2005), 17: Pietsch et al. (2007), 18: Garcia et al. (2000), 19: Kaaret (2002), 20: Williams et al. (2004), 21: Kong et al. (2002b), 22: Williams et al. (2005a), 23: Di Stefano et al. (2004), 24: Barnard et al. (2003), 25: Shaw Greening et al. (2009), 26: Pietsch et al. (2005b), 27: Stiele et al. (2008), 28: Trudolyubov et al. (2002) ; t: transient, v: variable, sv: spectrally variable, r: recurrent, d: dipping, z: Z-source candidate; BH: black hole, XRN: X-ray nova, XRT: X-ray transient, LMXB: low mass X-ray binary, NS: neutron star; numbers indicate the variability given by the corresponding paper.

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