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dc.contributor.authorBERNHARD, Sabrina
dc.contributor.authorBALZER, Arnim
hal.structure.identifierCentre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG]
dc.contributor.authorBRUN, Francois
dc.date.issued2017
dc.date.conference2016-07-11
dc.description.abstractEnCertain classes of astrophysical phenomena at high energies are known to be irregularly variable or of transient character, related to sources such as GRBs, AGN, or binary systems. Due to nonoptimized analysis schemes for transient searches at short timescales, some of those phenomena might have escaped proper characterization in the present H.E.S.S. analysis chains.In order to test the performance of our transient analysis capabilities, a module was developed to inject fake events into real data files. In that way a finite level of variability can be added to data from real sources to mimic characteristic variability patterns.Accordingly, this tool allows us to investigate the sensitivity limits of the analysis chains as a function of a variety of assumptions, such as different time profiles or spectral transitions, and to study performance and reliability for application in short-time transient searches with H.E.S.S.
dc.language.isoen
dc.source.titleAIP Conf.Proc.
dc.title.enSensitivity and performance simulations for transient phenomena in the H.E.S.S. analysis framework
dc.typeCommunication dans un congrès
dc.identifier.doi10.1063/1.4969001
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]
bordeaux.page070004
bordeaux.volume1792
bordeaux.issue1
bordeaux.countryDE
bordeaux.title.proceedingAIP Conf.Proc.
bordeaux.conference.cityHeidelberg
bordeaux.peerReviewednon
hal.identifierhal-01554379
hal.version1
hal.invitednon
hal.proceedingsoui
hal.conference.end2016-07-15
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01554379v1
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