Candidate isolated neutron stars in the 4XMM-DR10 catalog of X-ray sources
Michela Rigoselli, Sandro Mereghetti, Caterina Tresoldi

TL;DR
This study searches the 4XMM-DR10 X-ray catalog for isolated neutron stars emitting thermal X-ray radiation, identifying four promising candidates for further multiwavelength follow-up.
Contribution
It introduces a new method combining spectral analysis and catalog cross-correlations to identify potential thermally-emitting isolated neutron stars in a large X-ray source catalog.
Findings
Four candidate isolated neutron stars identified.
Spectral and variability analysis highlights promising sources.
Candidates warrant further multiwavelength observations.
Abstract
Most isolated neutron stars have been discovered thanks to the detection of their pulsed non-thermal emission, at wavelengths spanning from radio to gamma-rays. However, if the beamed non-thermal radiation does not intercept our line of sight or it is too faint or absent, isolated neutron stars can also be detected through their thermal emission, which peaks in the soft X-ray band and is emitted nearly isotropically. In the past thirty years, several thermally-emitting isolated neutron stars have been discovered thanks to X-ray all-sky surveys, observations targeted at the center of supernova remnants, or as serendipitous X-ray sources. Distinctive properties of these relatively rare X-ray sources are very soft spectra and high ratios of X-ray to optical flux. The recently released 4XMM-DR10 catalog contains more than half a million X-ray sources detected with the XMM-Newton telescope…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Geophysics and Sensor Technology · Seismic Waves and Analysis
