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A temporal analysis has been performed on a sample of 100 bright gamma-ray bursts (GRBs) with T90<2s from the BATSE current catalog. The GRBs were denoised using a median filter and subjected to an automated pulse selection algorithm as an…

Astrophysics · Physics 2009-11-07 S. McBreen , F. Quilligan , B. McBreen , L. Hanlon , D. Watson

A comprehensive temporal analysis has been performed on the 319 brightest GRBs with T90>2s from the BATSE current catalog. The rise times, fall times, full-widths at half maximum (FWHM), pulse amplitudes and pulse areas were measured and…

Astrophysics · Physics 2009-11-07 F. Quilligan , B. McBreen , L. Hanlon , S. McBreen , K. J. Hurley , D. Watson

In order to better understand the physical origin of short duration gamma-ray bursts (GRBs), we perform time-resolved spectral analysis on a sample of 70 pulses in 68 short GRBs with burst duration $T_{90}\lesssim2$ s detected by the…

High Energy Astrophysical Phenomena · Physics 2020-07-22 Hüsne Dereli-Bégué , Asaf Pe'er , Felix Ryde

The light curves of Gamma-Ray Bursts (GRBs) are believed to result from internal shocks reflecting the activity of the GRB central engine. Their temporal deconvolution can reveal potential differences in the properties of the central…

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 analyze the temporal structure of long ((T_{90}>2sec)) and short ((T_{90}<2sec)) BATSE bursts. We find that: (i) In many short bursts (\delta t_{min}/T\ll 1) (where (\delta t_{min}) is the shortest pulse). This indicates that short…

Astrophysics · Physics 2009-11-06 E. Nakar , T. Piran

Currently, the best available probe of the early phase of gamma-ray burst (GRB) jet attributes is the prompt gamma-ray emission, in which several intrinsic and extrinsic variables determine GRB pulse evolution. Bright, usually complex…

Astrophysics · Physics 2009-11-10 J. P. Norris , J. T. Bonnell , D. Kazanas , J. D. Scargle , J. Hakkila , T. W. Giblin

We demonstrate that distinguishable gamma-ray burst pulses exhibit similar behaviors as evidenced by correlations among the observable pulse properties of duration, peak luminosity, fluence, spectral hardness, energy-dependent lag, and…

High Energy Astrophysical Phenomena · Physics 2015-05-27 Jon Hakkila , Robert D. Preece

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

The temporal properties of a sample of 498 bright gamma-ray bursts (GRBs) with durations between 0.05 s and 674 s were analysed. The large range in duration (T90) is accompanied by a similarly large range in the median values of the pulse…

Astrophysics · Physics 2009-11-07 S. McBreen , B. McBreen , F. Quilligan , L. Hanlon

We analyze BATSE 64-ms data for long gamma-ray bursts (T90 > 2.6 s), exploring the relationships between spectral lag, duration, and the number of distinct pulses per burst, Npulses. We measure durations using a brightness-independent…

Astrophysics · Physics 2009-11-06 Jay P. Norris , Jeffrey D. Scargle , Jerry T. Bonnell

Using the data acquired in the Time To Spill (TTS) mode for long gamma-ray bursts (GRBs) collected by the Burst and Transient Source Experiment on board the Compton Gamma Ray Observatory (BATSE/CGRO), we have carefully measured spectral…

Astrophysics · Physics 2009-11-10 L. Chen , Y. Q. Lou , M. Wu , J. L. Qu , S. M. Jia , X. J. Yang

Gamma-ray bursts (GRBs) show different behaviours and trends in their spectral evolution. One of the methods used to understand the physical origin of these behaviours is to study correlation between the spectral fit parameters. In this…

High Energy Astrophysical Phenomena · Physics 2020-06-09 Hüsne Dereli Bégué , Hoi-Fung Yu , Felix Ryde

We have investigated the bimodal distribution of the duration of BATSE gamma-ray bursts (GRBs) by analyzing light curves of 64 ms time resolution. We define the average pulse width of GRBs from the auto-correlation function of GRB profiles.…

Astrophysics · Physics 2007-05-23 Wenfei Yu , Tipei Li , Mei Wu

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…

Astrophysics · Physics 2009-10-31 Andrew Lee , Elliott D. Bloom , Vahe Petrosian

Using a theoretical model describing pulse shapes, we have clarified the relations between the observed pulses and their corresponding timescales, such as the angular spreading time, the dynamic time as well as the cooling time. We find…

Astrophysics · Physics 2008-11-26 Zhibin Zhang , G. Z. Xie , J. G. Deng , B. T. Wei

Correlations among pulse properties in the prompt emission of long GRBs can potentially be used as cosmological distance indicators to estimate redshifts of GRBs to which these pulses belong. We demonstrate application of this technique to…

High Energy Astrophysical Phenomena · Physics 2009-06-25 Jon Hakkila , P. Chris Fragile , Timothy W. Giblin

We analyze a sample of bright long bursts and find that the pulses duration have a lognormal distribution while the intervals between pulses have an excess of long intervals (relative to lognormal distribution). This excess can be explained…

Astrophysics · Physics 2009-11-06 Ehud Nakar , Tsvi Piran

We present a simple, semi-analytical model to explain GRB temporal and spectral properties in the context of the internal shock model. Each individual pulse in the temporal profiles is produced by the deceleration of fast moving material by…

Astrophysics · Physics 2009-11-07 Frederic Daigne , Robert Mochkovitch

Gamma-ray bursts (GRBs) are widely believed to be from massive collapsars and/or compact binary mergers, which accordingly, would generate long and short GRBs, respectively. The details on this classification scheme have been in constant…

High Energy Astrophysical Phenomena · Physics 2022-03-02 Shuai Zhang , Lang Shao , Bin-Bin Zhang , Jin-Hang Zou , Hai-Yuan Sun , Yu-Jie Yao , Lin-Lin Li
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