000354859 001__ 354859
000354859 005__ 20250210102614.0
000354859 0247_ $$2doi$$a10.1103/PhysRevD.109.083019
000354859 0247_ $$2ISSN$$a2470-0010
000354859 0247_ $$2ISSN$$a2470-0037
000354859 0247_ $$2ISSN$$a2470-0029
000354859 0247_ $$2WOS$$aWOS:001221668800007
000354859 0247_ $$2datacite_doi$$a10.15120/GSI-2024-01292
000354859 037__ $$aGSI-2024-01292
000354859 041__ $$aEnglish
000354859 082__ $$a530
000354859 1001_ $$00000-0001-8276-997X$$aAbbar, Sajad$$b0$$eCorresponding author
000354859 245__ $$aApplication of neural networks for the reconstruction of supernova neutrino energy spectra following fast neutrino flavor conversions
000354859 260__ $$aRidge, NY$$bAmerican Physical Society$$c2024
000354859 3367_ $$2DRIVER$$aarticle
000354859 3367_ $$2DataCite$$aOutput Types/Journal article
000354859 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$bjournal$$mjournal$$s1739176808_410936
000354859 3367_ $$2BibTeX$$aARTICLE
000354859 3367_ $$2ORCID$$aJOURNAL_ARTICLE
000354859 3367_ $$00$$2EndNote$$aJournal Article
000354859 500__ $$aPublished by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license.
000354859 536__ $$0G:(DE-HGF)POF4-899$$a899 - ohne Topic (POF4-899)$$cPOF4-899$$fPOF IV$$x0
000354859 536__ $$0G:(EU-Grant)885281$$aKILONOVA - Probing r-process nucleosynthesis through its electromagnetic signatures (885281)$$c885281$$fERC-2019-ADG$$x1
000354859 536__ $$0G:(GEPRIS)390783311$$aDFG project G:(GEPRIS)390783311 - EXC 2094: ORIGINS: Vom Ursprung des Universums bis zu den ersten Bausteinen des Lebens (390783311)$$c390783311$$x2
000354859 536__ $$0G:(GEPRIS)283604770$$aDFG project G:(GEPRIS)283604770 - SFB 1258: Neutrinos und Dunkle Materie in der Astro- und Teilchenphysik (NDM) (283604770)$$c283604770$$x3
000354859 588__ $$aDataset connected to CrossRef, Journals: repository.gsi.de
000354859 693__ $$0EXP:(DE-Ds200)no_experiment-20200803$$1EXP:(DE-Ds200)theory-20200803$$5EXP:(DE-Ds200)no_experiment-20200803$$atheory$$eno experiment theory work (theory)$$x0
000354859 7001_ $$00000-0003-4960-8706$$aWu, Meng-Ru$$b1
000354859 7001_ $$0P:(DE-Ds200)OR10336$$aXiong, Zewei$$b2$$ugsi
000354859 773__ $$0PERI:(DE-600)2844732-3$$a10.1103/PhysRevD.109.083019$$gVol. 109, no. 8, p. 083019$$n8$$p083019$$tPhysical review / D$$v109$$x2470-0010$$y2024
000354859 8564_ $$uhttps://repository.gsi.de/record/354859/files/PhysRevD.109.083019.pdf$$yOpenAccess
000354859 8564_ $$uhttps://repository.gsi.de/record/354859/files/PhysRevD.109.083019.pdf?subformat=pdfa$$xpdfa$$yOpenAccess
000354859 909CO $$ooai:repository.gsi.de:354859$$popenaire$$popen_access$$pdriver$$pVDB$$pec_fundedresources$$pdnbdelivery
000354859 9101_ $$0I:(DE-Ds200)20121206GSI$$6P:(DE-Ds200)OR10336$$aGSI Helmholtzzentrum für Schwerionenforschung GmbH$$b2$$kGSI
000354859 9131_ $$0G:(DE-HGF)POF4-899$$1G:(DE-HGF)POF4-890$$2G:(DE-HGF)POF4-800$$3G:(DE-HGF)POF4$$4G:(DE-HGF)POF$$aDE-HGF$$bProgrammungebundene Forschung$$lohne Programm$$vohne Topic$$x0
000354859 9141_ $$y2024
000354859 915__ $$0StatID:(DE-HGF)0150$$2StatID$$aDBCoverage$$bWeb of Science Core Collection$$d2024-02-05
000354859 915__ $$0StatID:(DE-HGF)0160$$2StatID$$aDBCoverage$$bEssential Science Indicators$$d2024-02-05
000354859 915__ $$0StatID:(DE-HGF)1230$$2StatID$$aDBCoverage$$bCurrent Contents - Electronics and Telecommunications Collection$$d2024-02-05
000354859 915__ $$0LIC:(DE-HGF)CCBY4$$2HGFVOC$$aCreative Commons Attribution CC BY 4.0
000354859 915__ $$0StatID:(DE-HGF)0600$$2StatID$$aDBCoverage$$bEbsco Academic Search$$d2024-02-05
000354859 915__ $$0StatID:(DE-HGF)1150$$2StatID$$aDBCoverage$$bCurrent Contents - Physical, Chemical and Earth Sciences$$d2024-02-05
000354859 915__ $$0StatID:(DE-HGF)9905$$2StatID$$aIF >= 5$$bPHYS REV D : 2022$$d2024-02-05
000354859 915__ $$0StatID:(DE-HGF)0200$$2StatID$$aDBCoverage$$bSCOPUS$$d2024-02-05
000354859 915__ $$0StatID:(DE-HGF)0113$$2StatID$$aWoS$$bScience Citation Index Expanded$$d2024-02-05
000354859 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess
000354859 915__ $$0StatID:(DE-HGF)0571$$2StatID$$aDBCoverage$$bSCOAP3 sponsored Journal$$d2024-02-05
000354859 915__ $$0StatID:(DE-HGF)0100$$2StatID$$aJCR$$bPHYS REV D : 2022$$d2024-02-05
000354859 915__ $$0StatID:(DE-HGF)0020$$2StatID$$aNo Peer Review$$bASC$$d2024-02-05
000354859 915__ $$0StatID:(DE-HGF)0300$$2StatID$$aDBCoverage$$bMedline$$d2024-02-05
000354859 915__ $$0StatID:(DE-HGF)0199$$2StatID$$aDBCoverage$$bClarivate Analytics Master Journal List$$d2024-02-05
000354859 9201_ $$0I:(DE-Ds200)KNA-20160901OR396$$kKNA$$lNukleare Astrophysik & Struktur$$x0
000354859 980__ $$ajournal
000354859 980__ $$aVDB
000354859 980__ $$aUNRESTRICTED
000354859 980__ $$aI:(DE-Ds200)KNA-20160901OR396
000354859 9801_ $$aFullTexts