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A very bright, very hot, and very long flaring event from the M Dwarf Binary system DG CVn

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Figure

Figure 1. Comprehensive light curve of the event as seen in soft X-rays, UVOT bands, and ground-based optical photometry
Figure 2. X-ray spectra at the time of the trigger (top panels, BAT only) and during the initial ∼200 s after the XRT and BAT both were on source (bottom panels).The left panels show spectra fit with thermal models; right panels show thesame spectra fit wit
Table 1
Table 2
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