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dc.contributor.authorUrsi, Alessandro
dc.contributor.authorTavani, Marco
dc.contributor.authorVerrecchia, Francesco
dc.contributor.authorMarisaldi, Martino
dc.contributor.authorArgan, Andrea
dc.contributor.authorTrois, Alessio
dc.contributor.authorTempesta, Patrizio
dc.date.accessioned2020-04-28T14:07:59Z
dc.date.available2020-04-28T14:07:59Z
dc.date.issued2019
dc.PublishedUrsi A, Tavani M, Verrecchia F, Marisaldi M, Argan A, Trois A, Tempesta. A New AGILE MCAL Configuration to Detect Gamma-Ray Bursts and Sub-threshold Events in the Multimessenger Era. Astrophysical Journal. 2019;871(1):27eng
dc.identifier.issn0004-637Xen_US
dc.identifier.issn1538-4357en_US
dc.identifier.urihttps://hdl.handle.net/1956/22042
dc.description.abstractStarting in 2016 August, the onboard software configuration of the Astrorivelatore Gamma ad Immagini LEggero (AGILE) MiniCALorimeter (MCAL) was modified in order to increase the instrument trigger capabilities for the detection of short duration high-energy transients, such as weak gamma-ray sub-threshold events and short gamma-ray bursts. MCAL is a nonimaging, all-sky detector, operating in the energy range 0.4–100 MeV. This change was carried out in order to make AGILE more competitive in the detection of electromagnetic counterparts to gravitational wave events revealed by the Laser Interferometer Gravitational-Wave Observatory/Virgo experiments. In the 22 months from 2016 August to 2018 May, the new adopted MCAL-GW configuration substantially enhanced the number of MCAL onboard triggers, increasing the total acquisition time of the instrument, and resulted in the detection of 52 bursts, 40 of which have been confirmed by the InterPlanetary Network.en_US
dc.language.isoengeng
dc.publisherAmerican Astronomical Societyen_US
dc.titleA New AGILE MCAL Configuration to Detect Gamma-Ray Bursts and Sub-threshold Events in the Multimessenger Eraen_US
dc.typePeer reviewed
dc.typeJournal article
dc.date.updated2019-11-22T09:33:57Z
dc.description.versionpublishedVersionen_US
dc.rights.holderCopyright 2019. The American Astronomical Society. All rights reserved.en_US
dc.identifier.doihttps://doi.org/10.3847/1538-4357/aaf28f
dc.identifier.cristin1726909
dc.source.journalAstrophysical Journal


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