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Spectral characterization of the non-thermal X-ray emission of gamma-ray pulsars

We report on a detailed spectral characterization of the non-thermal X-ray emission for a large sample of gamma-ray pulsars in the second Fermi-LAT catalogue. We outline the criteria adopted for the selection of our sample, its completeness, and critically describe different approaches to estimate the spectral shape and flux of pulsars. We perform a systematic modelling of the pulsars' X-ray spectra using archival observations with XMM-Newton, Chandra, and NuSTAR and extract the corresponding non-thermal X-ray spectral distributions. This set of data is made available online and is useful to confront with predictions of theoretical models.

preprint2019arXivOpen access
Francesco Coti ZelatiDiego F. TorresJian LiDaniele Vigano
astro-ph.HE
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Open access4 authors1 topic
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Francesco Coti ZelatiDiego F. TorresJian LiDaniele Vigano

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