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.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.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.language.iso | en | en_US |
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.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 |
dc.privacy.showsubmitter | false | |
dc.status.ispeerreviewed | true | |
dc.description.accreditation | Web of Science | en_US |