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A blazar as the likely counterpart to 4FGL J0647.7−4418 instead of a gamma-ray binary
External Source
chorus
Document Type
Version of Record
Authors
Josep Martí (Departamento de Física (EPSJ), Universidad de Jaén, Campus Las Lagunillas s/n Ed. A3, E-23071 Jaén, Spain)
Estrella Sánchez-Ayaso (Department of Integrated Sciences and Center for Advanced Studies in Physics, Mathematics and Computation, University of Huelva, E-21007 Huelva, Spain)
Pedro L Luque-Escamilla (Departamento de Ingeniería Mecánica y Minera (EPSJ), Universidad de Jaén, Campus Las Lagunillas s/n Ed. A3, E-23071 Jaén, Spain)
Josep M Paredes (Departament de Física Quàntica i Astrofísica, Institut de Ciències del Cosmos, Universitat de Barcelona, IEEC-UB, Martí i Franquès 1, E-08028 Barcelona, Spain)
Valentí Bosch-Ramon (Departament de Física Quàntica i Astrofísica, Institut de Ciències del Cosmos, Universitat de Barcelona, IEEC-UB, Martí i Franquès 1, E-08028 Barcelona, Spain)
Robin H D Corbet (University of Maryland, Baltimore County, and X-ray Astrophysics Laboratory, Code 662 NASA Goddard Space Flight Center, Greenbelt Rd., MD 20771, USA)
Date Acquired
October 19, 2024
Publication Date
November 1, 2020
Publication Information
Publication: Monthly Notices of the Royal Astronomical Society
Publisher: Oxford University Press (OUP)
Volume: 492
Issue: 3
Issue Publication Date: January 3, 2020
ISSN: 0035-8711
e-ISSN: 1365-2966
DOI: 10.1093/mnras/staa072
Funding Number(s)
funding: AYA2016-76012-C3-1-P
funding: MDM-2014-0369
funding: NNX15AU83G
Distribution Limits
Public

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