Fig. 3
Swift/XRT results for the confirmed neutron star LMXB AX J1754.2–2754. Left: the X-ray light curve observed in 2008 July–August (binned per satellite orbit). Right: the average X-ray spectrum obtained by summing all available data (2007 July–2008 August). The solid line represents the best-fit result to an absorbed powerlaw model and the bottom plot indicates the data to model ratio of the fit.
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