Rapid flaring in GRB 070125

Adria C. Updike, Dieter H. Hartmann, Peter A. Milne, Grant G. Williams, Joshua B. Haislip

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

GRB 070125 was one of the brightest afterglows observed to date. We report on the characteristics of this burst, and focus on a well-resolved re-brightening episode observed by the Bok telescope about one day after the trigger. We conclude that the flare is indicative of an energy injection episode, increasing the flux by 56%.

Original languageEnglish (US)
Title of host publicationGamma-Ray Bursts 2007 - Proceedings of the Santa Fe Conference
Pages232-236
Number of pages5
DOIs
StatePublished - Dec 1 2008
EventSanta Fe Conference on Gamma-Ray Bursts 2007, GRB 2007 - Santa Fe, NM, United States
Duration: Nov 5 2007Nov 9 2007

Publication series

NameAIP Conference Proceedings
Volume1000
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Other

OtherSanta Fe Conference on Gamma-Ray Bursts 2007, GRB 2007
CountryUnited States
CitySanta Fe, NM
Period11/5/0711/9/07

Keywords

  • Visible (390-750 nm)

ASJC Scopus subject areas

  • Physics and Astronomy(all)

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  • Cite this

    Updike, A. C., Hartmann, D. H., Milne, P. A., Williams, G. G., & Haislip, J. B. (2008). Rapid flaring in GRB 070125. In Gamma-Ray Bursts 2007 - Proceedings of the Santa Fe Conference (pp. 232-236). (AIP Conference Proceedings; Vol. 1000). https://doi.org/10.1063/1.2943451