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V404 Cygni with Fermi-LAT

Harvey, Max; Rulten, Cameron B; Chadwick, Paula M

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Authors

Max Harvey



Abstract

We revisit the well-studied outburst of the low-mass X-ray binary (LMXB) system V404 Cygni, and claims of γ-ray excesses observed with the Fermi-LAT instrument. Upon analysing an 11.5 yr data set with the 8-yr LAT point source catalogue and 8-yr background models, we find no evidence to suggest that there is high energy γ-ray emission during the outburst period (or at any other time) from V404 Cygni. This is due to the proximity of V404 Cygni to the γ-ray emitting blazar B2023+336, a luminous source approximately 0.3○ away, which causes source confusion at the position of V404 Cygni, the luminous γ-ray background, and the use of older background models and catalogues in previous studies.

Journal Article Type Article
Acceptance Date Jul 18, 2021
Online Publication Date Jul 22, 2021
Publication Date 2021-10
Deposit Date Oct 29, 2021
Publicly Available Date Nov 10, 2021
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Royal Astronomical Society
Peer Reviewed Peer Reviewed
Volume 506
Issue 4
Pages 6029-6038
DOI https://doi.org/10.1093/mnras/stab2097
Public URL https://durham-repository.worktribe.com/output/1227000
Related Public URLs https://arxiv.org/abs/2107.09395

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Copyright Statement
This article has been accepted for publication in Monthly notices of the Royal Astronomical Society. ©: 2021 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.






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