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XMM Newton observation of the anomalous X ray pulsar 4U 0142+61

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Figure

Fig. 1. Pulse profile of 4U 0142+61 in the energy range 0.3−10 keV.
Table 1. Phase averaged spectral fits. Best fit parameters for an absorbed power law (PL) and a bremsstrahlung (BREMS) continuum, withits 2respect to the EPIC-pn
Fig. 4. Results of phase resolved spectroscopy for a blackbody pluspower law. The 0.5units of 10power law model

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