The Large Magellanic Cloud with the Cherenkov Telescope Array

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MetadadosDescriçãoIdioma
Autor(es): dc.contributorCtr Invest Energet Medioambientales & Tecnol-
Autor(es): dc.contributorUniversidade Estadual Paulista (Unesp)-
Autor(es): dc.contributorUniv Nova Gor-
Autor(es): dc.contributorNatl Acad Sci Ukraine-
Autor(es): dc.creatorBernardos, Maria Isabel-
Autor(es): dc.creatorBenito, Maria [UNESP]-
Autor(es): dc.creatorIocco, Fabio [UNESP]-
Autor(es): dc.creatorMangano, Salvatore-
Autor(es): dc.creatorSergijenko, Olga-
Autor(es): dc.creatorKarukes, Ekaterina [UNESP]-
Autor(es): dc.creatorYang, Lili-
Autor(es): dc.creatorCTA Consortium-
Autor(es): dc.creatorDeVincenzi, M.-
Autor(es): dc.creatorCapone, A.-
Autor(es): dc.creatorMorselli, A.-
Data de aceite: dc.date.accessioned2022-02-22T00:09:37Z-
Data de disponibilização: dc.date.available2022-02-22T00:09:37Z-
Data de envio: dc.date.issued2020-12-09-
Data de envio: dc.date.issued2020-12-09-
Data de envio: dc.date.issued2019-01-01-
Fonte completa do material: dc.identifierhttp://dx.doi.org/10.1051/epjconf/201920901021-
Fonte completa do material: dc.identifierhttp://hdl.handle.net/11449/196499-
Fonte: dc.identifier.urihttp://educapes.capes.gov.br/handle/11449/196499-
Descrição: dc.descriptionThe Large Magellanic Cloud (LMC) is a spiral galaxy, satellite of the Milky way with a high star formation activity. It represents a unique laboratory for studying an extended and spatially resolved star-forming galaxy through gamma-ray observatories. Therefore, the LMC survey is one of the key science projects for the Cherenkov Telescope Array (CTA), the next-generation ground-based gamma-ray observatory. In this document we present the work performed over the last year by the CTA working group dedicated to the LMC, in order to offer a first characterization of the LMC at TeV energies. We have performed detectability forecasts based on the expected CTA performance for all sources in the region of interest of the LMC with known emission at GeV energies and above. Based on previous observations made by Fermi-LAT and H.E.S.S. we have characterized all point sources, extended sources and diffuse emission produced by cosmic-ray propagation, extrapolating their spectra to CTA energies. Finally, we have characterized the signal expected by different annihilation mechanisms of dark matter (DM) particles within the LMC, computing the detection sensitivity curve for this target in the cross-section-to-mass plane.-
Descrição: dc.descriptionCtr Invest Energet Medioambientales & Tecnol, Madrid, Spain-
Descrição: dc.descriptionUniv Estadual Paulista, Inst Fis Teor, ICTP South Amer Inst Fundamental Res, Sao Paulo, SP, Brazil-
Descrição: dc.descriptionUniv Nova Gor, Nova Gorica, Slovenia-
Descrição: dc.descriptionNatl Acad Sci Ukraine, Kiev, Ukraine-
Descrição: dc.descriptionUniv Estadual Paulista, Inst Fis Teor, ICTP South Amer Inst Fundamental Res, Sao Paulo, SP, Brazil-
Formato: dc.format4-
Idioma: dc.languageen-
Publicador: dc.publisherE D P Sciences-
Relação: dc.relation7th Roma International Conference On Astroparticle Physics (ricap18)-
???dc.source???: dc.sourceWeb of Science-
Título: dc.titleThe Large Magellanic Cloud with the Cherenkov Telescope Array-
Aparece nas coleções:Repositório Institucional - Unesp

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