Goldstein, Adam 2013 BATSE 5B的伽马暴谱的catalog

主要内容:
给出了2145个BATSE暴的19000个谱，一个暴可以分时段有多个谱。分别用五种不同的谱进行了拟合，得到了相应的参数。

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Title:		The BATSE 5B Gamma-Ray Burst Spectral Catalog
Authors:		Goldstein, Adam; Preece, Robert D.; Mallozzi, Robert S.; Briggs, Michael S.; Fishman, Gerald J.; Kouveliotou, Chryssa; Paciesas, William S.; Burgess, J. Michael
Affiliation:		AA(University of Alabama in Huntsville, 320 Sparkman Drive, Huntsville, AL 35899, USA), AB(University of Alabama in Huntsville, 320 Sparkman Drive, Huntsville, AL 35899, USA), AC(Deceased.), AD(University of Alabama in Huntsville, 320 Sparkman Drive, Huntsville, AL 35899, USA), AE(Space Science Office, VP62, NASA/Marshall Space Flight Center, Huntsville, AL 35812, USA), AF(Space Science Office, VP62, NASA/Marshall Space Flight Center, Huntsville, AL 35812, USA), AG(Universities Space Research Association, 320 Sparkman Drive, Huntsville, AL 35805, USA), AH(University of Alabama in Huntsville, 320 Sparkman Drive, Huntsville, AL 35899, USA)
Publication:		The Astrophysical Journal Supplement, Volume 208, Issue 2, article id. 21, 30 pp. (2013). (ApJS Homepage)
Publication Date:		10/2013
Origin:		IOP
Astronomy Keywords:		gamma-ray burst: general, methods: data analysis
DOI:		10.1088/0067-0049/208/2/21
Bibliographic Code:		2013ApJS..208...21G

Abstract

We present systematic spectral analyses of gamma-ray bursts (GRBs) detected with the Burst and Transient Source Experiment (BATSE) on board the Compton Gamma-Ray Observatory during its entire nine years of operation. This catalog contains two types of spectra extracted from 2145 GRBs, and fitted with five different spectral models resulting in a compendium of over 19,000 spectra. The models were selected based on their empirical importance to the spectral shape of many GRBs, and the analysis performed was devised to be as thorough and objective as possible. We describe in detail our procedures and criteria for the analyses, and present the bulk results in the form of parameter distributions. This catalog should be considered an official product from the BATSE Science Team, and the data files containing the complete results are available from the High-Energy Astrophysics Science Archive Research Center (HEASARC).

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