Fig. 1

Absorbed flux measurements of the CCO in HESS J1731−347 in the 0.5–10 keV energy range performed with different instruments. The error bars indicate only statistical errors. For the data point of Chandra 2010 taken from Halpern & Gotthelf (2010a), no error bar is available. The latest observations analyzed in this work are marked as XMM-Newton 2013a and XMM-Newton 2013b. The horizontal dotted line indicates the averaged flux of the three XMM-Newton observations (2007, 2013a, and 2013b) performed in the same imaging mode.
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