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Time-dependent search for neutrino emission from X-ray binaries with the ANTARES telescope

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Figure

Figure 1. Light curves for 4U 1705-440 as seen by Swift/BAT, RXTE/ASM and MAXI during the studied period
Table 1. List of 33 X-ray binaries with significant flares selected for this analysis.
Table 2. List of the studied flaring periods and the satellite used (R: Rossi; S: Swift; M: MAXI).
Table 3. List of 8 X-ray binaries with hardness transition states reported in Astronomer’s Telegram.
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