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The observed pulsar flux in the 0.2-3 keV energy range is $\\sim 10^{-14} \\, {\\rm erg \\, cm}^{-2} \\, {\\rm s}^{-1}$, which results in the recording of $\\sim 600$ source counts with the EPIC pn and MOS detectors. The X-ray radiation is dominated by nonthermal radiation and is well described by both a single power-law model (PL) and a sum of blackbody and power-law emission (BB+PL). 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