Kodama 2008 Yonetoku关系定宇宙学参数

主要内容:
方法回归到典型的定距离的方法：在假定Yonetoku关系正确的基础上，首先用和超新星一样距离的伽玛暴定标，然后延伸到红移大于超新星的地方，得到红移和距离的关系。

精彩摘抄:
距离和红移的关系，蓝色的距离来自超新星，红色的来自Yonetoku关系。

文章信息:

· arXiv e-print (arXiv:0802.3428)

· References in the Article

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Title:		Gamma-Ray Bursts in $1.8 <>
Authors:		Kodama, Yoshiki; Yonetoku, Daisuke; Murakami, Toshio; Tanabe, Sachiko; Tsutsui, Ryo; Nakamura, Takashi
Publication:		eprint arXiv:0802.3428
Publication Date:		02/2008
Origin:		ARXIV
Keywords:		Astrophysics
Comment:		4 pages, 4 figures, submitted to MNRAS
Bibliographic Code:		2008arXiv0802.3428K

Abstract

We calibrated the peak energy-peak luminosity relation of GRBs (so called Yonetoku relation) using 33 events with the redshift $z <> Bibtex entry for this abstract Preferred format for this abstract (see Preferences)