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Related papers: Explaining the Gamma Ray Burst Lag/Luminosity and …

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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

Simple hardness ratios are found to be a good estimator for the spectral peak energy in Gamma-Ray Bursts (GRBs). Specifically, a high correlation strength is found between the $\nu F_{\nu}$ peak in the spectrum of BATSE GRBs, $\epo$, and…

High Energy Astrophysical Phenomena · Physics 2018-02-05 Amir Shahmoradi , Robert J. Nemiroff

There are several lines of evidence indicating that the ultra-relativistic outflows powering gamma-ray bursts (GRBs) are collimated into narrow jets. However, these are indirect, and the jet structure is rather poorly constrained. What is…

High Energy Astrophysical Phenomena · Physics 2010-12-24 Jonathan Granot , Enrico Ramirez-Ruiz

The relation between the $\gamma$-ray and the emission line luminosities for a sample of 36 $\gamma$-ray loud blazars is investigated; an apparent correlation between them, $L_{\gamma} \propto L_{Line}^{0.69\pm0.11}$, with a correlation…

Astrophysics · Physics 2007-05-23 J. H. Fan

We use a homogeneous sample of gamma-ray bursts (GRB) extracted from 5.9 years of BATSE DISCLA data (astro-ph/9908190) and a variety of broken power-law luminosity functions to derive GRB luminosities and space densities. Luminosity…

Astrophysics · Physics 2009-10-31 Maarten Schmidt

Kouveliotou et al. (1993) recently confirmed that gamma-ray bursts are bimodal in duration. In this paper we compute the statistical properties of the short ($\le 2$~s) and long ($>2$~s) bursts using a method of analysis that makes no…

Astrophysics · Physics 2009-10-22 Shude Mao , Ramesh Narayan , Tsvi Piran

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

Continued study of the BATSE catalog verifies previously-identified correlations between pulse lag and pulse duration and corresponding anti-correlations between both properties and pulse peak flux for a large sample of Long GRB pulses; the…

High Energy Astrophysical Phenomena · Physics 2009-06-25 Jon Hakkila , Renata S. Cumbee

It is postulated in Einstein's relativity that the speed of light in vacuum is a constant for all observers. However, the effect of quantum gravity could bring an energy dependence of light speed, and a series of studies on high-energy…

High Energy Astrophysical Phenomena · Physics 2023-05-17 Jie Zhu , Bo-Qiang Ma

Using 220 Gamma-Ray Burst (GRB) redshifts and luminosities derived from the luminosity-variability relationship of Fenimore & Ramirez-Ruiz (2000), we show that there exists a significant correlation between the GRB luminosity and redshift.…

Astrophysics · Physics 2009-11-07 Nicole M. Lloyd-Ronning , Chris L. Fryer , Enrico Ramirez-Ruiz

We review five studies of the gamma-ray burst (GRB) luminosity function that are based on one or more of the proposed luminosity criteria, i.e., variability, spectral lag and spectral hardness. A comparison between the resulting luminosity…

Astrophysics · Physics 2007-05-23 Maarten Schmidt

Gamma-ray bursts (GRB) are extreme events. They are crudely classified into two groups based on their duration, namely the short and long bursts. Such a classification has proven to be useful to determine their progenitors: the merger of…

High Energy Astrophysical Phenomena · Physics 2015-03-17 Hüsne Dereli

Using the Euclidean value of <V/Vmax> as a cosmological distance indicator, we derive the isotropic-equivalent characteristic peak luminosity of gamma-ray bursts both longer and shorter than 2 s. The short bursts have essentially the same…

Astrophysics · Physics 2009-11-07 Maarten Schmidt

Gamma Ray Bursts (GRBs) visible up to very high redshift have become attractive targets as potential new distance indicators. It is still not clear whether the relations proposed so far originate from an unknown GRB physics or result from…

High Energy Astrophysical Phenomena · Physics 2015-02-24 Maria Giovanna Dainotti , Roberta Del Vecchio , Shigehiro Nagataki , Salvatore Capozziello

Recently proposed correlations between the energetics of Gamma-Ray Bursts (GRB) and their spectral properties, namely the peak energy of their prompt emission, are found to account for the observed fluence distribution of all `bright' BATSE…

Astrophysics · Physics 2007-05-23 Z. Bosnjak , A. Celotti , F. Longo , G. Barbiellini

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

If Gamma-ray Bursts (GRBs) are generally associated with supernovae like 1998bw, a relatively wide intrinsic luminosity function is implied, which indicates the existence of a large amount of undetected dim bursts, and a much higher…

Astrophysics · Physics 2007-05-23 H. Che

Intrinsic variability was searched for in arrival times of six gamma-ray bursts (GRBs) at high energies -- between 30 MeV and 2 GeV -- detected by the Fermi satellite's Large Area Telescope (LAT). The GRBs were selected from the Fermi LAT…

High Energy Astrophysical Phenomena · Physics 2024-07-31 E. Casey Aldrich , Robert J. Nemiroff

Gamma-ray observations have revealed strong variability in blazar luminosities in the gamma-ray band over time scales as short as minutes. We show, for the first time, that the correlation of the spectrum with intensity is consistent with…

High Energy Astrophysical Phenomena · Physics 2021-08-18 N. E. Canac , K. N. Abazajian , T. Tajima , T. Ebisuzaki , S. Horiuchi

Rapid optical transient events can be hard to detect because of the limited number of photons they produce. I discuss a method of inferring the presence of fast, chaotic variability in photometry using the normalized autocorrelation…

Instrumentation and Methods for Astrophysics · Physics 2025-07-03 Brian C. Lacki