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Fig. 3.


LX and LX/Lbol vs. spectral type for J0331−27 (flare peak luminosity and upper limit on the quiescent luminosity), compared with the other UCDs for which X-ray data are available (from Stelzer et al. 2006a; Williams et al. 2014; Cook et al. 2014 and references therein; Robrade et al. 2010; Gupta et al. 2011).

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