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dc.contributor.authorBersier, D.
dc.contributor.authorJAPELJ, J.
dc.contributor.authorKENNEA, J.
dc.contributor.authorKOPAC, D.
dc.contributor.authorKOUVELIOTOU, C.
dc.contributor.authorKURODA, D.
dc.contributor.authorLevan, A.
dc.contributor.authorMalesani, D.
dc.contributor.authorMARSHALL, F.
dc.contributor.authorNOUSEK, J.
dc.contributor.authorO'Brien, P.
dc.contributor.authorOsborne, J. P.
dc.contributor.authorPagani, C.
dc.contributor.authorPage, K. L.
dc.contributor.authorPage, M.
dc.contributor.authorPERRI, M.
dc.contributor.authorPRITCHARD, T.
dc.contributor.authorROMANO, P.
dc.contributor.authorSAITO, Y.
dc.contributor.authorSBARUFATTI, B.
dc.contributor.authorSALVATERRA, R.
dc.contributor.authorSteele, I.
dc.contributor.authorTanvir, N.
dc.contributor.authorVianello, G.
dc.contributor.authorWEIGAND, B.
dc.contributor.authorWiersema, K.
dc.contributor.authorDe Pasquale, Massımılıano
dc.contributor.authorTAGLIAFERRI, G.
dc.contributor.authorCUSUMANO, G.
dc.contributor.authorEvans, P. A.
dc.contributor.authorGHIRLANDA, G.
dc.contributor.authorGHISELLINI, G.
dc.contributor.authorGUIDORZI, C.
dc.contributor.authorKobayashi, S.
dc.contributor.authorKuin, P.
dc.contributor.authorMANGANO, V.
dc.contributor.authorOates, S.
dc.contributor.authorSAKAMOTO, T.
dc.contributor.authorSERINO, M.
dc.contributor.authorVirgili, F.
dc.contributor.authorZHANG, B. -B.
dc.contributor.authorBARTHELMY, S.
dc.contributor.authorBeardmore, A.
dc.contributor.authorBERNARDINI, M. G.
dc.contributor.authorBURROWS, D.
dc.contributor.authorCALDERONE, G.
dc.contributor.authorCAPALBI, M.
dc.contributor.authorChiang, J.
dc.contributor.authorD'ELIA, V.
dc.contributor.authorFUGAZZA, D.
dc.contributor.authorMASELLI, A.
dc.contributor.authorMELANDRI, A.
dc.contributor.authorNAVA, L.
dc.contributor.authorMundell, C. G.
dc.contributor.authorKAWAI, N.
dc.contributor.authorCampana, S.
dc.contributor.authorCOVINO, S.
dc.contributor.authorCUMMINGS, J. R.
dc.contributor.authorLA PAROLA, V.
dc.contributor.authorD'AVANZO, P.
dc.contributor.authorYATSU, Y.
dc.contributor.authorYOSHII, T.
dc.contributor.authorGEHRELS, N.
dc.contributor.authorGOMBOC, A.
dc.contributor.authorHarrison, R.
dc.contributor.authorHANAYAMA, H.
dc.date.accessioned2021-03-03T13:57:29Z
dc.date.available2021-03-03T13:57:29Z
dc.date.issued2014
dc.identifier.citationMASELLI A., MELANDRI A., NAVA L., Mundell C. G. , KAWAI N., Campana S., COVINO S., CUMMINGS J. R. , CUSUMANO G., Evans P. A. , et al., "GRB 130427A: A Nearby Ordinary Monster", SCIENCE, cilt.343, sa.6166, ss.48-51, 2014
dc.identifier.issn0036-8075
dc.identifier.otherav_36fb75f2-f475-4610-bd1b-ea60efd207e0
dc.identifier.othervv_1032021
dc.identifier.urihttp://hdl.handle.net/20.500.12627/41092
dc.identifier.urihttps://doi.org/10.1126/science.1242279
dc.description.abstractLong-duration gamma-ray bursts (GRBs) are an extremely rare outcome of the collapse of massive stars and are typically found in the distant universe. Because of its intrinsic luminosity (L similar to 3 x 10(53) ergs per second) and its relative proximity (z = 0.34), GRB 130427A reached the highest fluence observed in the gamma-ray band. Here, we present a comprehensive multiwavelength view of GRB 130427A with Swift, the 2-meter Liverpool and Faulkes telescopes, and by other ground-based facilities, highlighting the evolution of the burst emission from the prompt to the afterglow phase. The properties of GRB 130427A are similar to those of the most luminous, high-redshift GRBs, suggesting that a common central engine is responsible for producing GRBs in both the contemporary and the early universe and over the full range of GRB isotropic energies.
dc.language.isoeng
dc.subjectDoğa Bilimleri Genel
dc.subjectTemel Bilimler
dc.subjectTemel Bilimler (SCI)
dc.subjectÇOK DİSİPLİNLİ BİLİMLER
dc.titleGRB 130427A: A Nearby Ordinary Monster
dc.typeMakale
dc.relation.journalSCIENCE
dc.contributor.departmentIstituto Nazionale Astrofisica , ,
dc.identifier.volume343
dc.identifier.issue6166
dc.identifier.startpage48
dc.identifier.endpage51
dc.contributor.firstauthorID103572


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