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Table 1.

Bright X-ray flares (Lx ≳ 1036 erg s−1) detected by INTEGRAL, Swift/BAT, MAXI, and long Suzaku and XMM-Newton observations of IGR J08408−4503 at lower luminosities.

Time Instrument Orbital Reference
(MJD) phase
52821.839 INTEGRAL 0.071 (a)
53870.770 INTEGRAL 0.980 (a)
58489.526 INTEGRAL 0.944 This work
53853.223 Swift/BAT 0.141 (b)
54012.613 Swift/BAT 0.843 (b)
54214.559 Swift/BAT 0.003 (b)
54652.887 Swift/BAT 0.932 (b)
54730.320 Swift/BAT 0.046 (b)
55071.953 Swift/BAT 0.843 (b)
55283.664 Swift/BAT 0.026 (b)
55798.035 Swift/BAT 0.923 (b)
56475.341 Swift/BAT 0.893 (c)
55914.029 MAXI 0.077 (d)
57640.955 MAXI 0.028 (d)
58451.443 MAXI 0.953 (d)
55176.746−55179.500 Suzaku −0.177 ≤ ϕ ≤ +0.112 (e)
54249.391−54249.918 XMM-Newton 0.653 ≤ ϕ ≤ 0.708 (f)

Notes. (a) Götz et al. (2007); (b) Romano et al. (2014b); (c) Romano et al. (2013); (d)List of the detection of transient sources reported in http://maxi.riken.jp/alert/novae/index.html; (e) Sidoli et al. (2010); (f) Bozzo et al. (2010).

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