Virgili, Francisco 2011 Swift/BAT-Fermi/GBM的谱的联合分析
主要内容:
可以得到新的E_p和谱指数等。
精彩摘抄:
文章信息:
· Find Similar Abstracts (with default settings below) - · arXiv e-print (arXiv:1112.4363)
- · References in the Article
- · Citations to the Article (1) (Citation History)
- · Refereed Citations to the Article
- · Also-Read Articles (Reads History)
- ·
- · Translate This Page
Title: | Spectral and temporal analysis of the joint Swift/BAT-Fermi/GBM GRB sample | |
Authors: | Virgili, Francisco; Qin, Ying; Zhang, Bing; Liang, Enwei | |
Publication: | eprint arXiv:1112.4363 | |
Publication Date: | 12/2011 | |
Origin: | ARXIV | |
Keywords: | Astrophysics - High Energy Astrophysical Phenomena | |
Comment: | 17 pages, 8 figures, 3 tables, MNRAS submitted | |
Bibliographic Code: | 2011arXiv1112.4363V |
Abstract
Using the gamma-ray bursts simultaneously detected by Swift/BAT and Fermi/GBM we perform a joint spectral and temporal analysis of the prompt emission data. Using derived spectral parameters, we confirm the rough correlation between the BAT-band photon index Gamma^BAT and the peak spectral energy E_peak. With the redshift known sub-sample, we derive the isotropic gamma-ray energy E_gamma,iso and confirm the E_gamma,iso - E_peak,rest relation, with a larger scatter than the Amati sample but consistent with another analysis by the GBM team. We also compare the T_90 values derived in the GBM band with those derived in the BAT band. We find that for long GRBs the BAT T_90 is usually longer than the GBM T_90, while for short GRBs the trend reverses. This is consistent with the soft/hard nature of long/short GRBs and suggests the importance of an energy-dependent temporal analysis of GRBs.Bibtex entry for this abstract Preferred format for this abstract (see Preferences) |
没有评论:
发表评论