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The neutron star in HESS J1731-347: Central compact objects as laboratories to study the equation of state of superdense matter
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3. Upper limits on the pulsed fraction. The XMM-Newton observations in imaging mode analyzed here permit a search for periodicity below the Nyquist frequency ... We note, however, that the analysis of the ~20 ksec tim[ing-mode data set upper limits without revealing pulsations]
No X-ray pulsations have been detected from the compact object in HESS J1731-347
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- https://arxiv.org/abs/1410.1055
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