Properties of Gamma‐Ray Burst Time Profiles Using Pulse Decomposition Analysis
Open Access
- 1 November 2000
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal Supplement Series
- Vol. 131 (1) , 1-19
- https://doi.org/10.1086/317364
Abstract
The time profiles of many gamma-ray bursts consist of distinct pulses, which offers the possibility of characterizing the temporal structure of these bursts using a relatively small set of pulse shape parameters. This pulse decomposition analysis has previously been performed on a small sample of bright, long bursts using binned data from BATSE, which comes in several data types, and on a sample of short bursts using the BATSE time-tagged event (TTE) data type. We have developed an interactive pulse-fitting program using the phenomenological pulse model of Norris et al. and a maximum-likelihood fitting routine. We have used this program to analyze the time-to-spill (TTS) data for all bursts observed by BATSE up through trigger number 2000, in all energy channels for which TTS data is available. This represents a total of 211 distinct bursts analyzed in one or more energy channels. We present statistical information on the attributes of pulses comprising these bursts, including relations between pulse characteristics in different energy channels and the evolution of pulse characteristics through the course of a burst. We carry out simulations to determine the biases that our procedures may introduce. We find that pulses tend to have shorter rise times than decay times, and tend to be narrower and peak earlier at higher energies. We also find that pulse brightness, pulse width, and pulse hardness ratios do not evolve monotonically within bursts, but that the ratios of pulse rise times to decay times tend to decrease with time within bursts.Keywords
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This publication has 14 references indexed in Scilit:
- On the Intrinsic and Cosmological Signatures in Gamma‐Ray Burst Time Profiles: Time DilationThe Astrophysical Journal Supplement Series, 2000
- Pulse Width Evolution in Gamma‐Ray Bursts: Evidence for Internal ShocksThe Astrophysical Journal, 2000
- Temporal evolution of the pulse width in GRBsAstronomy and Astrophysics Supplement Series, 1999
- The Third BATSE Gamma-Ray Burst CatalogThe Astrophysical Journal Supplement Series, 1996
- Attributes of Pulses in Long Bright Gamma-Ray BurstsThe Astrophysical Journal, 1996
- Determination of Distance from Time Dilation of Cosmological Gamma-Ray BurstsThe Astrophysical Journal, 1995
- Gamma-ray bursts are time-asymmetricThe Astrophysical Journal, 1994
- Identification of two classes of gamma-ray burstsThe Astrophysical Journal, 1993
- Prevalent properties of gamma-ray burst variabilityThe Astrophysical Journal, 1993
- Spectral evolution of pulse structures in gamma-ray burstsThe Astrophysical Journal, 1986