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dc.contributor.authorPless, Irwin A.
dc.date.accessioned2015-05-26T19:51:25Z
dc.date.available2015-05-26T19:51:25Z
dc.date.issued2015-03
dc.date.submitted2014-10
dc.identifier.issn1538-4357
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1721.1/97081
dc.description.abstractThe Large Volume Detector (LVD) has been continuously taking data since 1992 at the INFN Gran Sasso National Laboratory. The LVD is sensitive to neutrino bursts from gravitational stellar collapses with full detection probability over the Galaxy. We have searched for neutrino bursts in LVD data taken over 7,335 days of operation. No evidence of neutrino signals has been found between 1992 June and 2013 December. The 90% C.L. upper limit on the rate of core collapse and failed supernova explosions out to distances of 25 kpc is found to be 0.114 yr[superscript −1].en_US
dc.language.isoen_US
dc.publisherIOP Publishingen_US
dc.relation.isversionofhttp://dx.doi.org/10.1088/0004-637x/802/1/47en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceIOP Publishingen_US
dc.titleIMPLICATION FOR THE CORE-COLLAPSE SUPERNOVA RATE FROM 21 YEARS OF DATA OF THE LARGE VOLUME DETECTORen_US
dc.typeArticleen_US
dc.identifier.citationAgafonova, N. Y., M. Aglietta, P. Antonioli, V. V. Ashikhmin, G. Badino, G. Bari, R. Bertoni, et al. “IMPLICATION FOR THE CORE-COLLAPSE SUPERNOVA RATE FROM 21 YEARS OF DATA OF THE LARGE VOLUME DETECTOR.” The Astrophysical Journal 802, no. 1 (March 20, 2015): 47. © 2015 The American Astronomical Societyen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.mitauthorPless, Irwin A.en_US
dc.relation.journalThe Astrophysical Journalen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsAgafonova, N. Y.; Aglietta, M.; Antonioli, P.; Ashikhmin, V. V.; Badino, G.; Bari, G.; Bertoni, R.; Bressan, E.; Bruno, G.; Dadykin, V. L.; Dobrynina, E. A.; Enikeev, R. I.; Fulgione, W.; Galeotti, P.; Garbini, M.; Ghia, P. L.; Giusti, P.; Gomez, F.; Kemp, E.; Malgin, A. S.; Molinario, A.; Persiani, R.; Pless, I. A.; Porta, A.; Ryasny, V. G.; Ryazhskaya, O. G.; Saavedra, O.; Sartorelli, G.; Shakiryanova, I. R.; Selvi, M.; Trinchero, G. C.; Vigorito, C.; Yakushev, V. F.; Zichichi, A.en_US
dc.identifier.orcidhttps://orcid.org/0000-0002-4937-6514
mit.licensePUBLISHER_POLICYen_US
mit.metadata.statusComplete


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