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dc.contributor.authorAbe, H.
dc.contributor.authorAbe, S.
dc.contributor.authorAcciari, V.A.
dc.contributor.authorAniello, T.
dc.contributor.authorAnsoldi, S.
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dc.contributor.authorJin, W.
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dc.contributor.authorKertzman, M.
dc.contributor.authorKherlakian, M.
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dc.contributor.authorKumar, S.
dc.contributor.authorLang, M.J.
dc.contributor.authorLundy, M.
dc.contributor.authorMaier, G.
dc.contributor.authorMcGrath, C.E.
dc.contributor.authorMillis, J.
dc.contributor.authorMoriarty, P.
dc.contributor.authorMukherjee, R.
dc.contributor.authorO'Brien, S.
dc.contributor.authorOng, R.A.
dc.contributor.authorPark, N.
dc.contributor.authorPatel, S.R.
dc.contributor.authorPfrang, K.
dc.contributor.authorPohl, M.
dc.contributor.authorPueschel, E.
dc.contributor.authorQuinn, J.
dc.contributor.authorRagan, K.
dc.contributor.authorReynolds, P.T.
dc.contributor.authorRibeiro, D.
dc.contributor.authorRoache, E.
dc.contributor.authorRyan, J.L.
dc.contributor.authorSadeh, I.
dc.contributor.authorSaha, L.
dc.contributor.authorSantander, M.
dc.contributor.authorSembroski, G.H.
dc.contributor.authorShang, R.
dc.contributor.authorSplettstoesser, M.
dc.contributor.authorTak, D.
dc.contributor.authorTucci, J.V.
dc.contributor.authorWeinstein, A.
dc.contributor.authorWilliams, D.A.
dc.contributor.authorWilliamson, T.J.
dc.contributor.authorBosch-Ramon, V.
dc.contributor.authorCelma, C.
dc.contributor.authorLinares, Manuel
dc.contributor.authorRussell, D.M.
dc.contributor.authorSala, G.
dc.date.accessioned2023-02-03T14:04:55Z
dc.date.available2023-02-03T14:04:55Z
dc.date.created2023-01-13T09:14:31Z
dc.date.issued2022
dc.identifier.issn0035-8711
dc.identifier.urihttps://hdl.handle.net/11250/3048367
dc.description.abstractMAXI J1820+070 is a low-mass X-ray binary with a black hole (BH) as a compact object. This binary underwent an exceptionally bright X-ray outburst from 2018 March to October, showing evidence of a non-thermal particle population through its radio emission during this whole period. The combined results of 59.5 h of observations of the MAXI J1820+070 outburst with the H.E.S.S., MAGIC and VERITAS experiments at energies above 200 GeV are presented, together with Fermi-LAT data between 0.1 and 500 GeV, and multiwavelength observations from radio to X-rays. Gamma-ray emission is not detected from MAXI J1820+070, but the obtained upper limits and the multiwavelength data allow us to put meaningful constraints on the source properties under reasonable assumptions regarding the non-thermal particle population and the jet synchrotron spectrum. In particular, it is possible to show that, if a high-energy (HE) gamma-ray emitting region is present during the hard state of the source, its predicted flux should be at most a factor of 20 below the obtained Fermi-LAT upper limits, and closer to them for magnetic fields significantly below equipartition. During the state transitions, under the plausible assumption that electrons are accelerated up to ∼500 GeV, the multiwavelength data and the gamma-ray upper limits lead consistently to the conclusion that a potential HE and very-HE gamma-ray emitting region should be located at a distance from the BH ranging between 1011 and 1013 cm. Similar outbursts from low-mass X-ray binaries might be detectable in the near future with upcoming instruments such as CTA.en_US
dc.language.isoengen_US
dc.publisherOxford University Pressen_US
dc.titleGamma-ray observations of MAXI J1820+070 during the 2018 outbursten_US
dc.typeJournal articleen_US
dc.typePeer revieweden_US
dc.description.versionpublishedVersionen_US
dc.rights.holderCopyright 2022 The Author(s)en_US
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.doi10.1093/mnras/stac2686
dc.identifier.cristin2106162
dc.source.journalMonthly notices of the Royal Astronomical Societyen_US
dc.source.pagenumber4736-4751en_US
dc.identifier.citationMonthly notices of the Royal Astronomical Society. 2022, 517 (4), 4736-4751.en_US
dc.source.volume517en_US
dc.source.issue4en_US


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