Isolated neutron stars as Science Validation for XMM2ATHENA: Ensuring robust data for future X-ray Astronomy - Archive ouverte HAL
Communication Dans Un Congrès Année : 2024

Isolated neutron stars as Science Validation for XMM2ATHENA: Ensuring robust data for future X-ray Astronomy

Résumé

The discovery of radio-quiet, X-ray thermally emitting isolated neutron stars (XINSs) in the ROSAT All-Sky Survey revealed a previously overlooked component of the neutron star population. Advancements in X-ray instrumentation and the availability of deep, wide-area optical surveys now enable us to explore XINSs at fainter X-ray fluxes and greater distances. In this study, we investigated candidates selected from the 4XMM-DR9 catalogue using XMM-Newton, focusing on long-term flux stability, spectral characterisation, and astrometry. By leveraging resources from the XMM2ATHENA project -- including updated catalogues, multiwavelength characterisation and machine learning classification -- we refined our understanding of this sample of soft X-ray emitters. Our findings enhance the characterisation of XINS candidates, laying the groundwork for more targeted investigations and future catalogue searches.

Dates et versions

hal-04830392 , version 1 (11-12-2024)

Identifiants

Citer

Adriana Mancini Pires, Christian Motch, Axel Schwope, Iris Traulsen, Jean Ballet, et al.. Isolated neutron stars as Science Validation for XMM2ATHENA: Ensuring robust data for future X-ray Astronomy. 11th International Workshop on Astronomy and Relativistic Astrophysics, Sep 2024, Porto Alegre, Peru. ⟨10.1002/asna.20240116⟩. ⟨hal-04830392⟩
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