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X-ray dim isolated neutron star candidates from the eROSITA All-Sky Survey

Published online by Cambridge University Press:  27 February 2023

J. Kurpas Open the ORCID record for J. Kurpas [Opens in a new window] ,
A. Schwope ,
A. M. Pires Open the ORCID record for A. M. Pires [Opens in a new window]  and
F. Haberl
J. Kurpas
Affiliation:
Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, 14482 Potsdam, Germany
A. Schwope
Affiliation:
Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, 14482 Potsdam, Germany
A. M. Pires
Affiliation:
Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, 14482 Potsdam, Germany
F. Haberl
Affiliation:
Max-Planck-Institut für extraterrestrische Physik, Gießenbachstraße 1, 85748 Garching, Germany email: [email protected]
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Abstract

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After 2 years of continuous observations, the eROSITA All-Sky Survey bears the potential to build a complete sample of X-ray dim isolated neutron stars (XDINS). Making use of their soft X-ray emission and large X-ray-to-optical flux ratios, we selected a sample of ∼100 candidates detected down to a limiting flux of ∼10-13 erg s-1cm-2(0.2-2 keV). Follow-up observations of the best candidates will rule out possible contaminants. Updated source catalogues and screening algorithms will further improve our efficiency to identify new XDINS.

Keywords

stars: neutronsurveyspulsars: general
Type
Poster Paper
Information
Proceedings of the International Astronomical Union , Volume 16 , Symposium S363: Neutron Star Astrophysics at the Crossroads: Magnetars and the Multimessenger Revolution , June 2020 , pp. 345 - 346
Copyright
© The Author(s), 2023. Published by Cambridge University Press on behalf of International Astronomical Union

References

Høg, E., et al., 2000, A&A, 355, L27 Google Scholar
Keane, E. F., Kramer, M., 2008, MNRAS, 391, 2009.CrossRefGoogle Scholar
Pineau, F.-X., et al., 2017, A&A, 597, A89.Google Scholar
Pires, A. M., Motch, C., Janot-Pacheco, E., 2009, A&A, 504, 185.Google Scholar
Pires, A. M., Schwope, A. D., Motch, C., 2017, AN, 338, 213.Google Scholar
Predehl, P., et al., 2021, A&A, 647, A1.Google Scholar
Rigoselli, M., Mereghetti, S., Tresoldi, C., 2022, MNRAS, 509, 1217.Google Scholar
Viganò, D.,et al., 2013, MNRAS, 434, 123.CrossRefGoogle Scholar