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An improved redshift indicator for Gamma-Ray Bursts, based on the prompt emission
Pélangeon A., Atteia J.-L., Lamb D. Q., Ricker G. R.
http://hal.archives-ouvertes.fr/hal-00016624
Preprint, Working Paper, Document sans référence, etc.
Physique/Astrophysique/Cosmologie et astrophysique extra-galactique
Planète et Univers/Astrophysique
An improved redshift indicator for Gamma-Ray Bursts, based on the prompt emission
Alexandre Pélangeon () 1, Jean-Luc Atteia 1, Don Q. Lamb 2, George R. Ricker 3
1 :  Laboratoire d'Astrophysique de l'Observatoire Midi-Pyrénées (LATT)
http://webast.ast.obs-mip.fr
CNRS : UMR5572 – INSU – Observatoire Midi-Pyrénées – Université Paul Sabatier [UPS] - Toulouse III
14, avenue Edouard Belin 31400 Toulouse
France
2 :  Department of Astronomy and Astrophysics
University of Chicago
Chicago, IL 60637
États-Unis
3 :  Center for Space Research
Massachussetts Institute of Technology
Cambridge, MA 02139
États-Unis
We propose an improved version of the redshift indicator developed by Atteia (2003), which gets rid of the dependence on the burst duration and provides better estimates for high-redshift GRBs. We present the derivation and the definition of this redshift indicator, then its calibration with 17 GRBs with known redshifts detected by HETE-2 and 2 more detected by Konus-Wind. We also provide an estimation of the redshift for 59 bursts, and we finally discuss the redshift distribution of HETE-bursts and the possible other applications of this redshift indicator.
Anglais

gamma-rays:bursts
PACS: 95.85.Pw, PACS: 98.70.Rz
To appear in the proceedings of the 16th Annual October Astrophysics Conference in Maryland, "Gamma Ray Bursts in the Swift Era", Washington DC., November 29-December 2, 2005, 4 pages, 3 figures

the HETE Science Team

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aip-6s.clo(15.9 KB)
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pelangeon.tex(14.7 KB)
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pelangeon.ps(143.2 KB)
PDF
pelangeon.pdf(51.3 KB)