Predicting gamma-ray burster redshifts from their prompt emission properties

dc.contributor.author	Koen, Chris
dc.date.accessioned	2013-10-20T20:22:14Z
dc.date.available	2013-10-20T20:22:14Z
dc.date.issued	2010
dc.description.abstract	This paper presents a study of the relation between gamma-ray burster redshift and several of its prompt emission properties (spectral lag, light curve variability, peak energy, rise time and the peak bolometric flux Pbol). Simple predictors of log(1 + z) in terms of Pbol and the other indicators are derived. The typical scatter in the relations is 0.13 dex. An illustrative application to observations of GRB 090423 (z ∼ 8) is given.	en_US
dc.description.accreditation	Web of Science	en_US
dc.identifier.citation	Koen, C. (2010). Predicting gamma-ray burster redshifts from their prompt emission properties. Monthly Notices of the Royal Astronomical Society, 401: 1369–1374	en_US
dc.identifier.issn	0035-8711
dc.identifier.uri	http://hdl.handle.net/10566/774
dc.language.iso	en	en_US
dc.privacy.showsubmitter	false
dc.publisher	Oxford University Press	en_US
dc.rights	© 2010 copyright Oxford University Press. This file may be freely used for educational purposes, as long as it is not altered in any way. Acknowledgement of the authors and the source is required.
dc.source.uri	http://dx.doi.org/10.1111/j.1365-2966.2009.15737.x
dc.status.ispeerreviewed	true
dc.subject	Methods: statistical	en_US
dc.subject	Gamma-rays: bursts	en_US
dc.title	Predicting gamma-ray burster redshifts from their prompt emission properties	en_US
dc.type	Article	en_US

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