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.

星期五, 十一月 26, 2010

Sakamoto 2010 用伽马暴的观测来校正卫星

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Title:
Spectral Cross-calibration of the Konus-Wind, the Suzaku/WAM, and the Swift/BAT Data using Gamma-Ray Bursts
Authors:
Sakamoto, T.; Pal'shin, V.; Yamaoka, K.; Ohno, M.; Sato, G.; Aptekar, R.; Barthelmy, S.; Baumgartner, W.; Cummings, J.; Fenimore, E.; Frederiks, D.; Gehrels, N.; Golenetskii, S.; Krimm, H.; Markwardt, C.; Onda, K.; Palmer, D.; Parsons, A.; Stamatikos, M.; Sugita, S.; Tashiro, M.; Tueller, J.; Ukwatta, T.
Publication:
eprint arXiv:1011.1301
Publication Date:
11/2010
Origin:
ARXIV
Keywords:
Astrophysics - High Energy Astrophysical Phenomena
Comment:
82 pages, 88 figures, accepted for publication in PASJ
Bibliographic Code:
2010arXiv1011.1301S

Abstract

We report on the spectral cross-calibration results of the Konus-Wind, the Suzaku/WAM, and the Swift/BAT instruments using simultaneously observed gamma-ray bursts (GRBs). This is the first attempt to use simultaneously observed GRBs as a spectral calibration source to understand systematic problems among the instruments. Based on these joint spectral fits, we find that 1) although a constant factor (a normalization factor) agrees within 20% among the instruments, the BAT constant factor shows a systematically smaller value by 10-20% compared to that of Konus-Wind, 2) there is a systematic trend that the low-energy photon index becomes steeper by 0.1-0.2 and Epeak becomes systematically higher by 10-20% when including the BAT data in the joint fits, and 3) the high-energy photon index agrees within 0.2 among the instruments. Our results show that cross-calibration based on joint spectral analysis is an important step to understanding the instrumental effects which could be affecting the scientific results from the GRB prompt emission data.
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