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dc.contributor.authorWinslow, Lindley
dc.date.accessioned2022-05-05T14:53:02Z
dc.date.available2022-05-05T14:53:02Z
dc.date.issued2021
dc.identifier.urihttps://hdl.handle.net/1721.1/142360
dc.description.abstract<jats:title>Abstract</jats:title> <jats:p>The next core-collapse supernova in the Milky Way or its satellites will represent a once-in-a-generation opportunity to obtain detailed information about the explosion of a star and provide significant scientific insight for a variety of fields because of the extreme conditions found within. Supernovae in our galaxy are not only rare on a human timescale but also happen at unscheduled times, so it is crucial to be ready and use all available instruments to capture all possible information from the event. The first indication of a potential stellar explosion will be the arrival of a bright burst of neutrinos. Its observation by multiple detectors worldwide can provide an early warning for the subsequent electromagnetic fireworks, as well as signal to other detectors with significant backgrounds so they can store their recent data. The supernova early warning system (SNEWS) has been operating as a simple coincidence between neutrino experiments in automated mode since 2005. In the current era of multi-messenger astronomy there are new opportunities for SNEWS to optimize sensitivity to science from the next galactic supernova beyond the simple early alert. This document is the product of a workshop in June 2019 towards design of SNEWS 2.0, an upgraded SNEWS with enhanced capabilities exploiting the unique advantages of prompt neutrino detection to maximize the science gained from such a valuable event.</jats:p>en_US
dc.language.isoen
dc.publisherIOP Publishingen_US
dc.relation.isversionof10.1088/1367-2630/ABDE33en_US
dc.rightsCreative Commons Attribution 4.0 International Licenseen_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0en_US
dc.sourceIOP Publishingen_US
dc.titleSNEWS 2.0: A Next-Generation SuperNova Early Warning System for Multi-messenger Astronomyen_US
dc.typeArticleen_US
dc.identifier.citationWinslow, Lindley. 2021. "SNEWS 2.0: A Next-Generation SuperNova Early Warning System for Multi-messenger Astronomy." New Journal of Physics, 23 (3).
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physics
dc.relation.journalNew Journal of Physicsen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2022-05-05T14:45:32Z
dspace.orderedauthorsAl Kharusi, S; BenZvi, SY; Bobowski, JS; Bonivento, W; Brdar, V; Brunner, T; Caden, E; Clark, M; Coleiro, A; Colomer-Molla, M; Crespo-Anadón, JI; Depoian, A; Dornic, D; Fischer, V; Franco, D; Fulgione, W; Gallo Rosso, A; Geske, M; Griswold, S; Gromov, M; Haggard, D; Habig, A; Halim, O; Higuera, A; Hill, R; Horiuchi, S; Ishidoshiro, K; Kato, C; Katsavounidis, E; Khaitan, D; Kneller, JP; Kopec, A; Kulikovskiy, V; Lai, M; Lamoureux, M; Lang, RF; Li, HL; Lincetto, M; Lunardini, C; Migenda, J; Milisavljevic, D; McCarthy, ME; O Connor, E; O Sullivan, E; Pagliaroli, G; Patel, D; Peres, R; Pointon, BW; Qin, J; Raj, N; Renshaw, A; Roeth, A; Rumleskie, J; Scholberg, K; Sheshukov, A; Sonley, T; Strait, M; Takhistov, V; Tamborra, I; Tseng, J; Tunnell, CD; Vasel, J; Vigorito, CF; Viren, B; Virtue, CJ; Wang, JS; Wen, LJ; Winslow, L; Wolfs, FLH; Xu, XJ; Xu, Yen_US
dspace.date.submission2022-05-05T14:45:37Z
mit.journal.volume23en_US
mit.journal.issue3en_US
mit.licensePUBLISHER_CC
mit.metadata.statusAuthority Work and Publication Information Neededen_US


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