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Fig. B.6
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eROSITA LMC SN1987A data noise-weighted residuals. The columns represent, from left to right, the nwr in the three energy channels (νlow = 0.2 - 1.0, keV, νref = 1.0 - 2.0, keV, and νhi = 2.0 - 4.5, keV), while the rows correspond to the three telescope modules used in the reconstruction (TM1, TM3, TM4).
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