X-rays observations of a super-Chandrasekhar object reveal an ONe and a CO white dwarf merger product embedded in a putative SN Iax remnant

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Fig. A.4.

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Same as in Fig. A.3, but for EPIC MOS1 and MOS2 spectra obtained during two pointings. The histograms show the best-fitting model (fourth column in Table A.2 of a two-temperature plasma), and the residuals as signed contributions.

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