Different satellites - different GRB redshift distributions?

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dc.creatorBagoly, Z.
dc.creatorBalazs, L. G.
dc.creatorHorvath, I.
dc.creatorKelemen, J.
dc.creatorMeszaros, A.
dc.creatorVeres, P.
dc.creatorTusnady, G.
dc.date2008-12-31
dc.date.accessioned2026-07-07T12:31:55Z
dc.date.available2026-07-07T12:31:55Z
dc.descriptionThe measured redshifts of gamma-ray bursts (GRBs), which were first detected by the Swift satellite, seem to be bigger on average than the redshifts of GRBs detected by other satellites. We analyzed the redshift distribution of GRBs triggered and observed by different satellites (Swift[1], HETE2[2], BeppoSax, Ulyssses). After considering the possible biases significant difference was found at the p = 95.70% level in the redshift distributions of GRBs measured by HETE and the Swift.
dc.description2008 NANJING GAMMA-RAY BURST CONFERENCE. AIP Conference Proceedings, Volume 1065, pp. 119-122 (2008)
dc.identifierhttps://arxiv.org/abs/0901.0103
dc.identifierhttp://arxiv.org/abs/0901.0103
dc.identifierdoi:10.1063/1.3027895
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/216615
dc.subjectHigh Energy Astrophysical Phenomena
dc.titleDifferent satellites - different GRB redshift distributions?
dc.typetext

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