Matches in SemOpenAlex for { <https://semopenalex.org/work/W2024145854> ?p ?o ?g. }
- W2024145854 endingPage "1042" @default.
- W2024145854 startingPage "1034" @default.
- W2024145854 abstract "We predict the redshift distribution of long gamma-ray bursts (GRBs) with Monte Carlo simulations. Our improved analysis constrains free parameters with three kinds of observation: (i) the log N− log P diagram of Burst and Transient Source Experiment (BATSE) bursts; (ii) the peak energy distribution of bright BATSE bursts and (iii) the High Energy Transient Explorer (HETE2) fraction of X-ray rich GRBs and X-ray flashes. The statistical analysis of the Monte Carlo simulation results allows us to carefully study the impact of the uncertainties in the GRB intrinsic properties on the redshift distribution. The comparison with Swift data then leads to the following conclusions. The Amati relation should be intrinsic, if observationally confirmed by Swift. The progenitor and/or the GRB properties have to evolve to reproduce the high mean redshift of Swift bursts. Our results favour an evolution of the efficiency of GRB production by massive stars, that would be nearly six to seven times higher at z∼ 7 than at z∼ 2. We finally predict around 10 GRBs detected by Swift at redshift z > 6 for a 3-yr mission. These may be sufficient to open a new observational window over the high redshift Universe." @default.
- W2024145854 created "2016-06-24" @default.
- W2024145854 creator A5017961660 @default.
- W2024145854 creator A5031008643 @default.
- W2024145854 creator A5049387961 @default.
- W2024145854 date "2006-11-01" @default.
- W2024145854 modified "2023-09-25" @default.
- W2024145854 title "The redshift distribution of Swift gamma-ray bursts: evidence for evolution" @default.
- W2024145854 cites W1590054290 @default.
- W2024145854 cites W1913860194 @default.
- W2024145854 cites W1958465016 @default.
- W2024145854 cites W1965141332 @default.
- W2024145854 cites W1973609488 @default.
- W2024145854 cites W1986285672 @default.
- W2024145854 cites W2003271886 @default.
- W2024145854 cites W2005488289 @default.
- W2024145854 cites W2007649291 @default.
- W2024145854 cites W2011457240 @default.
- W2024145854 cites W2012360551 @default.
- W2024145854 cites W2015679879 @default.
- W2024145854 cites W2022693158 @default.
- W2024145854 cites W2030418871 @default.
- W2024145854 cites W2037932817 @default.
- W2024145854 cites W2039492307 @default.
- W2024145854 cites W2043830471 @default.
- W2024145854 cites W2049899114 @default.
- W2024145854 cites W2049935166 @default.
- W2024145854 cites W2060963248 @default.
- W2024145854 cites W2075303178 @default.
- W2024145854 cites W2086775208 @default.
- W2024145854 cites W2114800671 @default.
- W2024145854 cites W2131053676 @default.
- W2024145854 cites W2132505194 @default.
- W2024145854 cites W2147737716 @default.
- W2024145854 cites W2150427241 @default.
- W2024145854 cites W2151199556 @default.
- W2024145854 cites W2161977657 @default.
- W2024145854 cites W2168770294 @default.
- W2024145854 cites W3098151581 @default.
- W2024145854 cites W3099391734 @default.
- W2024145854 cites W3099616520 @default.
- W2024145854 cites W3099803470 @default.
- W2024145854 cites W3100326233 @default.
- W2024145854 cites W3104748836 @default.
- W2024145854 cites W3105165820 @default.
- W2024145854 cites W3105502586 @default.
- W2024145854 cites W3124688811 @default.
- W2024145854 doi "https://doi.org/10.1111/j.1365-2966.2006.10837.x" @default.
- W2024145854 hasPublicationYear "2006" @default.
- W2024145854 type Work @default.
- W2024145854 sameAs 2024145854 @default.
- W2024145854 citedByCount "119" @default.
- W2024145854 countsByYear W20241458542012 @default.
- W2024145854 countsByYear W20241458542013 @default.
- W2024145854 countsByYear W20241458542014 @default.
- W2024145854 countsByYear W20241458542015 @default.
- W2024145854 countsByYear W20241458542016 @default.
- W2024145854 countsByYear W20241458542017 @default.
- W2024145854 countsByYear W20241458542018 @default.
- W2024145854 countsByYear W20241458542020 @default.
- W2024145854 countsByYear W20241458542021 @default.
- W2024145854 countsByYear W20241458542022 @default.
- W2024145854 countsByYear W20241458542023 @default.
- W2024145854 crossrefType "journal-article" @default.
- W2024145854 hasAuthorship W2024145854A5017961660 @default.
- W2024145854 hasAuthorship W2024145854A5031008643 @default.
- W2024145854 hasAuthorship W2024145854A5049387961 @default.
- W2024145854 hasBestOaLocation W20241458541 @default.
- W2024145854 hasConcept C105795698 @default.
- W2024145854 hasConcept C116188536 @default.
- W2024145854 hasConcept C121332964 @default.
- W2024145854 hasConcept C1276947 @default.
- W2024145854 hasConcept C150846664 @default.
- W2024145854 hasConcept C17599544 @default.
- W2024145854 hasConcept C19499675 @default.
- W2024145854 hasConcept C33024259 @default.
- W2024145854 hasConcept C33923547 @default.
- W2024145854 hasConcept C44870925 @default.
- W2024145854 hasConcept C98444146 @default.
- W2024145854 hasConceptScore W2024145854C105795698 @default.
- W2024145854 hasConceptScore W2024145854C116188536 @default.
- W2024145854 hasConceptScore W2024145854C121332964 @default.
- W2024145854 hasConceptScore W2024145854C1276947 @default.
- W2024145854 hasConceptScore W2024145854C150846664 @default.
- W2024145854 hasConceptScore W2024145854C17599544 @default.
- W2024145854 hasConceptScore W2024145854C19499675 @default.
- W2024145854 hasConceptScore W2024145854C33024259 @default.
- W2024145854 hasConceptScore W2024145854C33923547 @default.
- W2024145854 hasConceptScore W2024145854C44870925 @default.
- W2024145854 hasConceptScore W2024145854C98444146 @default.
- W2024145854 hasIssue "3" @default.
- W2024145854 hasLocation W20241458541 @default.
- W2024145854 hasLocation W20241458542 @default.
- W2024145854 hasLocation W20241458543 @default.
- W2024145854 hasLocation W20241458544 @default.
- W2024145854 hasLocation W20241458545 @default.
- W2024145854 hasOpenAccess W2024145854 @default.
- W2024145854 hasPrimaryLocation W20241458541 @default.