伽玛暴(Gamma-Ray Burst)笔记。记录有关伽玛暴的新文章,另外也包括看的老文章、自己的想法、以及跟天文相关的一些东西。 Feel free to leave me a message by comments or by email.

星期二, 二月 26, 2008

Ukwatta 2008 高红移暴的辐射特性

主要内容:
把这些暴的T90, Epeak等画到一张图上。

精彩摘抄:


文章信息:

· arXiv e-print (arXiv:0802.3815)
· References in the Article
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Title:
Screening High-z GRBs with BAT Prompt Emission Properties
Authors:
Ukwatta, T. N.; Sakamoto, T.; Stamatikos, M.; Gehrels, N.; Dhuga, K. S.
Publication:
eprint arXiv:0802.3815
Publication Date:
02/2008
Origin:
ARXIV
Keywords:
Astrophysics
Comment:
4 pages, 4 figures, to be published in the proceedings of ''Gamma Ray Bursts 2007'', Santa Fe, New Mexico, November 5-9
Bibliographic Code:
2008arXiv0802.3815U

Abstract

Detecting high-z GRBs is important for constraining the GRB formation rate, and tracing the history of re-ionization and metallicity of the universe. Based on the current sample of GRBs detected by Swift with known redshifts, we investigated the relationship between red-shift, and spectral and temporal characteristics, using the BAT event-by-event data. We found red-shift trends for the peak-flux-normalized temporal width T90, the light curve variance, the peak flux, and the photon index in simple power-law fit to the BAT event data. We have constructed criteria for screening GRBs with high red-shifts. This will enable us to provide a much faster alert to the GRB community of possible high-z bursts.
Bibtex entry for this abstract Preferred format for this abstract (see Preferences)

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