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Related papers: Time Dilation of BATSE Gamma-ray Bursts

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Many of the important conclusions about Gamma-Ray Bursts follow from the distributions of various quantities such as peak flux or duration. We show that for astrophysical transients such as bursts, multiple selection thresholds can lead to…

Astrophysics · Physics 2009-10-28 Vahe Petrosian , Theodore T. Lee

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. We have used a pulse…

Astrophysics · Physics 2014-10-13 Andrew Lee , Elliott D. Bloom , Vahe Petrosian

Two tests for cosmological time dilation in $\gamma$-ray bursts -- the peak alignment and auto-correlation statistics -- involve averaging information near the times of peak intensity. Both tests require width corrections, assuming…

Astrophysics · Physics 2009-10-28 J. P. Norris , R. J. Nemiroff , J. T. Bonnell , J. D. Scargle

If gamma-ray bursters are at cosmological distances - as suggested by their isotropic distribution on the sky and by their number-intensity relation - then the burst profiles will be stretched in time, by an amount proportional to the…

The isotropic distribution of gamma-ray bursts as observed with the Burst and Transient Experiment (BATSE) strongly suggests that the bursts are at cosmological distances. At such distances, the expansion of the universe should redshift the…

Astrophysics · Physics 2009-10-28 Ed E. Fenimore , Joshua S. Bloom

The recent discovery that faint gamma-ray bursts are stretched in time relative to bright ones has been interpreted as support for cosmological distances: faint bursts have their durations redshifted relative to bright ones. It was pointed…

Astrophysics · Physics 2009-10-22 Ralph A. M. J. Wijers , Bohdan Paczyński

We present strong evidence of time stretching in the peak-to-peak time scales in the light curves of BATSE Gamma Ray Bursts (GRBs). Extensive tests are performed on artificially dilated bursts to verify that the procedure for extracting the…

Astrophysics · Physics 2009-10-30 Ming Deng , Bradley E. Schaefer

The recent discovery that faint gamma-ray bursts are stretched in time relative to bright ones has been interpreted as support for cosmological distances: faint bursts have their durations redshifted relative to bright ones. It was pointed…

Astrophysics · Physics 2007-05-23 Ralph A. M. J. Wijers , Bohdan Paczyński

We study the temporal asymmetry of over 600 bursts from the BATSE 3B catalog, encompassing a 200-fold range in peak flux. By comparing the rates of rise and fall of the flux near the highest burst peak, we find that about two-thirds of the…

Astrophysics · Physics 2009-10-28 Bennett Link , Richard Epstein

We study the power density spectrum (PDS) of light curves of the observed gamma-ray bursts (GRBs) to search for a direct signature for cosmological time dilation in the PDS statistics with the GRBs whose redshifts $z$'s are known. The…

Astrophysics · Physics 2009-11-06 Heon-Young Chang

The cosmological expansion cannot produce the reported correlations of the gamma-ray burst timescale and spectral energy with peak flux if the burst model reproduces the BATSE 3B peak-flux distribution for a non-evolving burst source…

Astrophysics · Physics 2009-10-30 J. J. Brainerd

A time dependent two-point correlation-function analysis of the BATSE 2B catalog finds no evidence of burst repetition. As part of this analysis, we discuss the effects of sky exposure on the observability of burst repetition and present…

Astrophysics · Physics 2016-08-30 J. J. Brainerd , C. A. Meegan , Michael S. Briggs , G. N. Pendleton , M. N. Brock

Gamma-Ray Bursts have been observed out to very high redshifts and provide time measures that are directly related to intrinsic time scales of the burst. Einstein's theory of relativity is quite definite that if the universe is expanding…

General Physics · Physics 2010-09-12 David F. Crawford

A simple test for time-asymmetry is devised and carried out on the brightest gamma-ray bursts detected by the Burst and Transient Source Experiment (BATSE) on board the {\it Compton} Gamma Ray Observatory. We show evidence that individual…

If $\gamma$-ray bursts are at cosmological distances, then not only their constituent pulses but also the intervals between pulses should be time-dilated. Unlike time-dilation measures of pulse emission, intervals would appear to require…

Astrophysics · Physics 2009-10-28 J. P. Norris , J. T. Bonnell , R. J. Nemiroff , J. D. Scargle

We have measured the T90 and T50 durations of bright and dim gamma-ray bursts (GRBs) detected by the Compton Gamma Ray Observatory's Burst and Transient Source Experiment (BATSE). The T90 (T50) duration is defined as the interval over which…

Norris et al. (1994) report that the temporal structure of faint gamma ray bursts is longer than that of bright bursts, as expected for time dilation in the cosmological models of burst origin. I show that the observed trends can easily be…

Astrophysics · Physics 2009-10-22 David Band

We study the evolution with redshift of three measures of gamma-ray burst (GRB) duration ($T_{\rm 90}$, $T_{\rm 50}$ and $T_{\rm R45}$) in a fixed rest frame energy band for a sample of 232 Swift/BAT detected GRBs. Binning the data in…

High Energy Astrophysical Phenomena · Physics 2015-06-22 O. M. Littlejohns , N. R. Butler

We present an analysis indicating that there is a correlation between the fluences and the durations of gamma-ray bursts, and provide arguments that this reflects a correlation between the total emitted energies and the intrinsic durations.…

Astrophysics · Physics 2015-06-02 Istvan Horvath , Lajos G. Balazs , Peter Meszaros , Zsolt Bagoly , Attila Meszaros

We argue that the distributions of both the intrinsic fluence and the intrinsic duration of the gamma-ray emission in gamma-ray bursts from the BATSE sample are well represented by log-normal distributions, in which the intrinsic dispersion…

Astrophysics · Physics 2007-05-23 L. G. Balazs , P. Meszaros , Z. Bagoly , I. Horvath , A. Meszaros
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