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Fig. 2

image

Combined XMM-Newton spectrum (all EPIC cameras) from the three observations fitted with a carbon atmosphere model (top) and fit residuals for the blackbody, the carbon atmosphere, and the hydrogen atmosphere models (from top to bottom). The null-hypothesis probabilities (P-values) yielded by the χ2-fits are indicated. The blackbody model leads to a statistically unacceptable fit.

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