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Fig. B.1.
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Chandra+ACIS upper limits to the x-ray luminosity of SN 2019wxt, compared to the X-ray lightcurve of the Type Ibn SN 2006jc. The Swift+XRT limit < 6.6 × 1041 erg s−1 at 0 d is more than two orders of magnitude shallower than the data plotted here, and hence not plotted.
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