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The ~100 net-count 0.3-7 keV spectrum obtained from $\\sim 30$ ksec Chandra exposure is best fit by a single power-law model with a photon index $\\Gamma=2.0\\pm0.2$ and no indication of an intrinsic absorber, implying a 3.6-72 keV rest-frame luminosity $L_{\\rm X}=(2.3^{+0.6}_{-0.5})\\times10^{46}$ erg s$^{-1}$. 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