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GRB 190114C in the nuclear region of an interacting galaxy A detailed host analysis using ALMA, the HST, and the VLT

dc.contributor.authorTanvir, N. R.
dc.contributor.authorde Ugarte Postigo, A.
dc.contributor.authorThone, C. C.
dc.contributor.authorMartin, S.
dc.contributor.authorJapelj, J.
dc.contributor.authorLevan, A. J.
dc.contributor.authorMichalowski, M. J.
dc.contributor.authorSelsing, J.
dc.contributor.authorKann, D. A.
dc.contributor.authorSchulze, S.
dc.contributor.authorPalmerio, J. T.
dc.contributor.authorVergani, S. D.
dc.contributor.authorDe Pasquale, M.
dc.contributor.authorBensch, K.
dc.contributor.authorCovino, S.
dc.contributor.authorD'Elia, V
dc.contributor.authorFruchter, A. S.
dc.contributor.authorFynbo, J. P. U.
dc.contributor.authorHartmann, D.
dc.contributor.authorHeintz, K. E.
dc.contributor.authorvan der Horst, A. J.
dc.contributor.authorIzzo, L.
dc.contributor.authorJakobsson, P.
dc.contributor.authorNg, K. C. Y.
dc.contributor.authorPerley, D. A.
dc.contributor.authorRossi, A.
dc.contributor.authorSbarufatti, B.
dc.contributor.authorSalvaterra, R.
dc.contributor.authorSanchez-Ramirez, R.
dc.contributor.authorWatson, D.
dc.contributor.authorXu, D.
dc.date.accessioned2021-03-05T08:02:52Z
dc.date.available2021-03-05T08:02:52Z
dc.identifier.citationde Ugarte Postigo A., Thone C. C. , Martin S., Japelj J., Levan A. J. , Michalowski M. J. , Selsing J., Kann D. A. , Schulze S., Palmerio J. T. , et al., "GRB 190114C in the nuclear region of an interacting galaxy A detailed host analysis using ALMA, the HST, and the VLT", ASTRONOMY & ASTROPHYSICS, cilt.633, 2020
dc.identifier.issn0004-6361
dc.identifier.otherav_96e89bf7-6ff0-43aa-ae5b-9fed3b1913db
dc.identifier.othervv_1032021
dc.identifier.urihttp://hdl.handle.net/20.500.12627/101576
dc.identifier.urihttps://doi.org/10.1051/0004-6361/201936668
dc.description.abstractContext. For the first time, very high energy emission up to the TeV range has been reported for a gamma-ray burst (GRB). It is still unclear whether the environmental properties of GRB 190114C might have contributed to the production of these very high energy photons, or if it is solely related to the released GRB emission.
dc.language.isoeng
dc.subjectUzay bilimi
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectTemel Bilimler
dc.subjectAstronomi ve Astrofizik
dc.subjectFizik
dc.subjectTemel Bilimler (SCI)
dc.titleGRB 190114C in the nuclear region of an interacting galaxy A detailed host analysis using ALMA, the HST, and the VLT
dc.typeMakale
dc.relation.journalASTRONOMY & ASTROPHYSICS
dc.contributor.departmentİstanbul Üniversitesi , ,
dc.identifier.volume633
dc.contributor.firstauthorID272963


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