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Related papers: Short Gamma-Ray Bursts with Extended Emission

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We present the results of our systematic search for extended emission components following initial short gamma-ray burst (GRB) spikes, using Burst and Transient Source Experiment (BATSE) observations. We performed the extended emission…

High Energy Astrophysical Phenomena · Physics 2013-01-17 Zahide Funda Bostanci , Yuki Kaneko , Ersin Gogus

We analyze pulse properties of Short gamma-ray bursts (GRBs) from a new catalog containing 434 pulses from 387 BATSE Time-Tagged Event (TTE) GRBs. Short GRB pulses exhibit correlated properties of duration, fluence, hardness, and amplitude,…

High Energy Astrophysical Phenomena · Physics 2018-03-28 Jon Hakkila , Istvan Horvath , Eric Hofesmann , Stephen Lesage

We report evidence from the 3B Catalogue that long ($T_{90} > 10$ s) and short ($T_{90} < 10$ s) gamma-ray bursts represent distinct source populations. Their spatial distributions are significantly different, with long bursts having…

Astrophysics · Physics 2009-10-28 J. I. Katz , L. M. Canel

Owing to lack of multiple components of prompt $\gamma$-ray emissions in short gamma-ray bursts (sGRBs), how these distinct components are correlated still keeps unclear. In this paper, we investigate the spectral and temporal properties of…

High Energy Astrophysical Phenomena · Physics 2022-01-26 X. J. Li , Z. B. Zhang , K. Zhang

Gamma-ray bursts (GRBs) divide into two classes: "long", which typically have initial durations of T90>2s, and "short", with durations of T90<2s (where T90 is the time to detect 90% of the observed fluence). Long bursts, which on average…

Astrophysics · Physics 2009-11-16 N. R. Tanvir , R. Chapman , A. J. Levan , R. S. Priddey

The Burst and Transient Source Experiment (BATSE) classifies cosmological gamma-ray bursts (GRBs) into short (less than 2 s) and long (over 2 s) events, commonly attributed to mergers of compact objects and, respectively, peculiar…

High Energy Astrophysical Phenomena · Physics 2015-06-23 Maurice H. P. M. van Putten , Gyeong Min Lee , Massimo Della Valle , Lorenzo Amati , Amir Levinson

We compare the spectral properties of 79 short and 79 long Gamma-Ray Bursts (GRBs) detected by BATSE and selected with the same limiting peak flux. Short GRBs have a low-energy spectral component harder and a peak energy slightly higher…

High Energy Astrophysical Phenomena · Physics 2009-11-13 G. Ghirlanda , L. Nava , G. Ghisellini , A. Celotti , C. Firmani

We present the results of the spectral analysis of a sample of short bright $\gamma$--ray bursts (GRB) detected by BATSE and compare them with the average and time resolved spectral properties of long bright bursts. While the spectral…

Astrophysics · Physics 2009-11-10 G. Ghirlanda , G. Ghisellini , A. Celotti

We study the spectra of short-bright GRBs detected by BATSE and compare them with the average and time resolved spectral properties of long-bright bursts. We confirm that short events are harder than long bursts, as already found from the…

Astrophysics · Physics 2009-11-10 G. Ghirlanda , G. Ghisellini , A. Celotti

Data from the 3B Catalogue suggest that short and long GRB are the results of different classes of events, rather than different parameter values within a single class: Short bursts have harder spectra in the BATSE bands, but chiefly long…

Astrophysics · Physics 2007-05-23 J. I. Katz , L. M. Canel

We analyze BATSE time-tagged event (TTE) data for short gamma-ray bursts (T90 duration < 2.6 s), studying spectral lag vs. peak flux and duration, as well as the number of distinct pulse structures per burst. Performing the…

Astrophysics · Physics 2009-11-06 J. P. Norris , J. D. Scargle , J. T. Bonnell

Some short GRBs are followed by longer extended emission, lasting anywhere from ~10 to ~100 s. These short GRBs with extended emission (EE) can possess observational characteristics of both short and long GRBs (as represented by GRB…

High Energy Astrophysical Phenomena · Physics 2015-08-07 Y. Kaneko , Z. F. Bostanci , E. Gogus , L. Lin

Evidence is growing for a class of gamma-ray bursts (GRBs) characterized by an initial ~0.1-1 s spike of hard radiation followed, after a ~3-10 s lull in emission, by a softer period of extended emission lasting ~10-100 s. In a few…

Astrophysics · Physics 2009-11-13 B. D. Metzger , E. Quataert , Todd A. Thompson

We report evidence from the 3B Catalogue that short (T_90 < 10 s) and long (T_90 > 10 s) GRB represent different populations and processes: Their spectral behavior is qualitatively different, with short bursts harder in the BATSE range, but…

Astrophysics · Physics 2016-08-30 J. I. Katz , L. M. Canel

The distribution of GRB durations is bimodal, but there is little additional evidence to support the division of GRBs into short and long classes. Based on simple hardness ratios, several studies have shown a tendency for longer GRBs to…

Astrophysics · Physics 2009-11-07 W. S. Paciesas , R. D. Preece , M. S. Briggs , R. S. Mallozzi

Extended emission is a mystery in short gamma-ray bursts (SGRBs). By making time resolved spectral analyses of brightest nine events observed by ${\it Swift}$ XRT, we obviously classify the early X-ray emission of SGRBs into two types. One…

High Energy Astrophysical Phenomena · Physics 2015-11-30 Yasuaki Kagawa , Daisuke Yonetoku , Tatsuya Sawano , Asuka Toyanago , Takashi Nakamura , Keitaro Takahashi , Kazumi Kashiyama , Kunihito Ioka

A comprehensive study is given to short gamma-ray bursts (sGRBs) in the third Swift/BAT GRB Catalog from December 2004 to July 2019. We examine in details the temporal properties of the three components in the prompt gamma-ray emission…

High Energy Astrophysical Phenomena · Physics 2021-03-17 X. J. Li , Z. B. Zhang , X. L. Zhang , H. Y. Zhen

We have carried out a detailed study of the morphology of gamma-ray bursts (GRBs) with time duration less than 100 ms that includes: (1) a fast-Fourier spectrum analysis, (2) a comparison with the Stern analysis of longer bursts, (3) an…

Astrophysics · Physics 2009-10-31 David B. Cline , Christina Matthey , Stanislaw Otwinowski

This paper reports statistically significant correlations between various burst parameters, observed in a sample of 156 GRBs belonging to BATSE 4B catalog with T90 less than 2 s. The number of subpulses in a burst is strongly correlated not…

Astrophysics · Physics 2007-05-23 Varsha Gupta , Patrick Das Gupta , P. N. Bhat

Preliminary results of our analysis on the extended emission of short/medium duration GRBs observed with Swift/BAT are presented. The Bayesian blocks algorithm is used to analyze the burst durations and the temporal structure of the…

Astrophysics · Physics 2009-11-13 Lin Lin , En-Wei Liang , Bin-Bin Zhang , Shuang Nan Zhang
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