2008/09/17 by A. Pélangeon, J. -L. Atteia, J. L. Atteia +38 · 3 citations
Physics and Astronomy · #Astrophysics #Computer science #Context (archaeology) #Frame (networking) #Gamma ray #Gamma-ray burst #Gamma-ray bursts and supernovae #Geography #Physics #Pulsars and Gravitational Waves Research #Sample (material) #Simple (philosophy) #Stellar, planetary, and galactic studies #Telecommunications #astro-ph
paper · pdf · doi:10.1051/0004-6361:200809709
published as Astron.Astrophys.491:157-171,2008 · 20 pages, 14 figures, 3 tables (editor version: 15 pages, 14 figures, tables 2 and 3 only available in electronic form at http://www.aanda.org)
openalex publication_date 2008/09/17 · arxiv created 2008/11/20 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Context. As a result of the numerous missions dedicated to the detection of Gamma-ray bursts (GRBs), the observed properties of these events are now well known. However, studying their parameters in the source frame is not simple since it requires having measurements of both the bursts' parameters and of their distances.