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The Complete Spectral Catalog of Bright BATSE Gamma-Ray Bursts

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arxiv astro-ph/0601188 v1 pith:35WGUEAC submitted 2006-01-09 astro-ph

Yuki Kaneko , Robert D. Preece , Michael S. Briggs , William S. Paciesas , Charles A. Meegan , David L. Band This is my paper
classification astro-ph
keywords spectralgrbsparametersbatseanalysisbrightburstcatalog
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We present a systematic spectral analysis of 350 bright GRBs observed with BATSE, with high spectral and temporal resolution. Our sample was selected from the complete set of 2704 BATSE GRBs, and included 17 short GRBs. To obtain well-constrained spectral parameters, four different photon models were fitted and the spectral parameters that best represent each spectrum were statistically determined. A thorough analysis was performed on 350 time-integrated and 8459 time-resolved burst spectra. Using the results, we compared time-integrated and time-resolved spectral parameters, and also studied correlations among the parameters and their evolution within each burst. The resulting catalog is the most comprehensive study of spectral properties of GRB prompt emission to date, and provides constraints with exceptional statistics on particle acceleration and emission mechanisms in GRBs.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Modeling Gamma-Ray Burst Spectra with Convolutional Neural Networks: Fast-Cooling Synchrotron Emission in a Decaying Magnetic Field

    astro-ph.HE 2026-06 unverdicted novelty 6.0 of 10

    CNN emulator for decaying magnetic field fast-cooling synchrotron spectra is trained on synthetic data and used in Bayesian fits to GRB 231020A, favoring the decaying-field model over the standard version.

  2. Tightening Bounds on Warm Dark Matter with High-Redshift Gamma-Ray Bursts

    astro-ph.HE 2026-07 conditional novelty 4.0 of 10

    Using the redshift distribution of 118 luminous Swift GRBs, warm dark matter particles are bounded to mx ≥ 1.3 keV at 95% CL (≥3.4 keV if GRBs exactly trace the SFR).

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