Isolated Neutron Stars as Science Validation for <scp>XMM2ATHENA</scp>: Ensuring Robust Data for Future X‐Ray Astronomy

ABSTRACT 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.

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Publication Details

Journal
Astronomische Nachrichten
Published
2024-11-26
DOI
https://doi.org/10.1002/asna.20240116
Primary Topic
Astrophysical Phenomena and Observations
Type
article
Field-Weighted Citation Impact
0.00

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article

Isolated Neutron Stars as Science Validation for XMM2ATHENA: Ensuring Robust Data for Future X‐Ray Astronomy

C. Motch, Sudip Chakraborty, N. A. Webb, D. Homan et al.
Astronomische Nachrichten
Astrophysical Phenomena and Observations
article

Isolated Neutron Stars as Science Validation for XMM2ATHENA: Ensuring Robust Data for Future X‐Ray Astronomy

C. Motch, Sudip Chakraborty, N. A. Webb, D. Homan, A. M. Pires, A. Schwope, A. Nebot Gómez-Morán, Hugo Tranin, J. Kurpas, Iris Traulsen, F.-X. Pineau, J. Ballet
article en

Abstract

ABSTRACT 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.

Astronomische NachrichtenVol. 346(3-4)
Centre National de la Recherche Scientifique (FR), Université Fédérale de Toulouse Midi-Pyrénées (FR), Chinese Academy of Sciences (CN), Université Paris Cité (FR), Commissariat à l'Énergie Atomique et aux Énergies Alternatives (FR), Université Paris-Saclay (FR), Leibniz Institute for Astrophysics Potsdam (DE), Observatoire astronomique de Strasbourg (FR), Astrophysique, Instrumentation et Modélisation (FR), CEA Paris-Saclay (FR), Institute of Geochemistry (CN)
European Commission, Chinese Academy of Sciences, Deutsches Zentrum für Luft- und Raumfahrt, National Key Research and Development Program of China, Institute of Geochemistry, Chinese Academy of Sciences
Openalex Percentile: Top 84%
Astrophysical Phenomena and Observations
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