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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