Deriving the redshift of distant galaxies with Gamma-Ray Burst transient edges

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dc.creatorFloc'h, E. Le
dc.creatorDuc, P. -A.
dc.creatorMirabel, I. F.
dc.date2002-11-12
dc.date.accessioned2026-07-07T02:06:10Z
dc.date.available2026-07-07T02:06:10Z
dc.descriptionCosmological Gamma-Ray Bursts (GRBs) offer a unique perspective to probe the evolution of distant galaxies. We discuss one of the multiple benefits of this approach, i.e. the detection of transient edges in the GRB prompt phase emission. These absorption features can be used to directly derive the redshift of GRBs and their host galaxies without the need of any optical spectroscopic follow-up.
dc.description2 pages (format A5), 1 figure, Proceedings SF2A-2002, Paris, ed. F. Combes and D. Barret, EDP-Sciences
dc.identifierhttps://arxiv.org/abs/astro-ph/0211254
dc.identifierhttp://arxiv.org/abs/astro-ph/0211254
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5331
dc.subjectAstrophysics
dc.titleDeriving the redshift of distant galaxies with Gamma-Ray Burst transient edges
dc.typetext

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