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I have used a sample of long Gamma Ray Bursts (GRBs) common to both \emph{Swift} and \emph{Fermi} to re-derive the parameters of the Yonetoku correlation. This allowed me to self-consistently estimate pseudo redshifts of all the bursts with…

High Energy Astrophysical Phenomena · Physics 2017-11-29 Debdutta Paul

We compute the luminosity function (LF) and the formation rate of long gamma ray bursts (GRBs) by fitting the observed differential peak flux distribution obtained by the BATSE satellite in three different scenarios: i) GRBs follow the…

Astrophysics · Physics 2009-11-11 R. Salvaterra , C. Chincarini

We study the luminosity function and formation rate of long gamma-ray bursts (GRBs) by using a maximum likelihood method. This is the first time this method is applied to a well-defined sample of GRBs that is complete in redshift. The…

High Energy Astrophysical Phenomena · Physics 2019-07-31 Guang-Xuan Lan , Hou-Dun Zeng , Jun-Jie Wei , Xue-Feng Wu

We compute the luminosity function (LF) and the formation rate of long gamma ray bursts (GRBs) by fitting the observed differential peak flux distribution obtained by the BATSE experiment in two different scenarios: i) the GRB luminosity…

Astrophysics · Physics 2015-05-13 R. Salvaterra , C. Guidorzi , S. Campana , G. Chincarini , G. Tagliaferri

The determination of luminosity function (LF) of gamma-ray bursts (GRBs) is of an important role for the cosmological applications of the GRBs, which is however hindered seriously by some selection effects due to redshift measurements. In…

High Energy Astrophysical Phenomena · Physics 2013-10-17 Wei-Wei Tan , Xiao-Feng Cao , Yun-Wei Yu

We use a sample of \textit{Swift} gamma-ray bursts (GRBs) to analyze the Amati and Yonetoku correlations. The first relation is between $E_{p,i}$, the intrinsic peak energy of the prompt GRB emission, and $E_{iso}$, the equivalent isotropic…

High Energy Astrophysical Phenomena · Physics 2016-11-18 Hannachi Zitouni , Nidhal Guessoum , Walid Jamil Azzam

We compute the luminosity function (LF) and the formation rate of long gamma ray bursts (GRBs) in three different scenarios: i) GRBs follow the cosmic star formation and their LF is constant in time; ii) GRBs follow the cosmic star…

We present a carefully selected sub-sample of Swift Long Gamma-ray Bursts (GRBs), that is complete in redshift. The sample is constructed by considering only bursts with favorable observing conditions for ground-based follow-up searches,…

We use the BD2 sample of gamma-ray bursts (GRBs) based on 5.9 years of BATSE DISCLA data with a variety of models of the luminosity function to derive characteristic GRB luminosities, space densities and redshift distributions. Previously…

Astrophysics · Physics 2009-10-31 Maarten Schmidt

In this catalog, we present the results of a systematic study of gamma-ray bursts (GRBs) with reliable redshift estimates detected in the triggered mode of the Konus-Wind (KW) experiment during the period from 1997 February to 2016 June.…

High Energy Astrophysical Phenomena · Physics 2017-11-30 A. Tsvetkova , D. Frederiks , S. Golenetskii , A. Lysenko , P. Oleynik , V. Pal'shin , D. Svinkin , M. Ulanov , T. Cline , K. Hurley , R. Aptekar

We study the redshift evolution of the luminosity function (LF) and redshift selection effect of long gamma-ray bursts (LGRBs). The method is to fit the observed peak flux and redshift distributions, simultaneously. To account for the…

High Energy Astrophysical Phenomena · Physics 2015-10-14 W. W. Tan , F. Y. Wang

We compute the intrinsic isotropic peak luminosity function (LF) and formation rate of long gamma-ray bursts (LGRBs) using a novel approach. We complement a standard log\,$N$\,--\,log\,$P$ brightness distribution and $V_{\mathrm{max}}$…

High Energy Astrophysical Phenomena · Physics 2015-06-22 E. J. Howell , D. M. Coward , G. Stratta , B. Gendre , H. Zhou

Gamma-ray bursts (GRBs) are the most violent explosions in the Universe and can be used to explore the properties of high-redshift universe. It is believed that the long GRBs are associated with the deaths of massive stars. So it is…

High Energy Astrophysical Phenomena · Physics 2015-05-27 H. Yu , F. Y. Wang , Z. G. Dai , K. S. Cheng

Starting from the Swift sample we define a complete sub-sample of 58 bright long Gamma Ray Bursts (GRB), 55 of them (95%) with a redshift determination, in order to characterize their properties. Our sample (BAT6) allows us to study the…

High Energy Astrophysical Phenomena · Physics 2013-09-11 R. Salvaterra , S. Campana , S. Covino , P. D'Avanzo , G. Ghirlanda , G. Ghisellini , A. Melandi , G. Tagliaferri , L. Nava , S. Vergani

Luminosity function and event rate of Gamma-Ray Bursts (GRBs) are easily biased by the instrument and selection effects. We select 115 Fermi/GBM GRBs with good spectra fitted by a smoothly broken power-law function. The $\tau$-statistic…

High Energy Astrophysical Phenomena · Physics 2025-07-23 Yang Liu , Zhi-Bin Zhang , Xiao-Fei Dong , Long-Biao Li , Xiu-Yun Du

The cosmic formation rate of long Gamma Ray Bursts (LGRBs) encodes the evolution, across cosmic times, of their progenitors' properties and of their environment. The LGRB formation rate and the luminosity function, with its redshift…

High Energy Astrophysical Phenomena · Physics 2022-06-15 G. Ghirlanda , R. Salvaterra

In the Second part of The Konus-Wind Catalog of Gamma-Ray Bursts with Known Redshifts (first part: Tsvetkova et al. 2017; T17), we present the results of a systematic study of gamma-ray bursts (GRBs) with reliable redshift estimates…

High Energy Astrophysical Phenomena · Physics 2021-02-19 A. Tsvetkova , D. Frederiks , D. Svinkin , R. Aptekar , T. L. Cline , S. Golenetskii , K. Hurley , A. Lysenko , A. Ridnaia , M. Ulanov

The cosmic evolution of gamma-ray burst (GRB) luminosity is essential for revealing the GRB physics and for using GRBs as cosmological probes. We investigate the luminosity evolution of long GRBs with a large sample of 258 {\em Swift}/BAT…

High Energy Astrophysical Phenomena · Physics 2016-04-06 Can-Min Deng , Xiang-Gao Wang , Bei-Bei Guo , Rui-Jing Lu , Yuan-Zhu Wang , Jun-Jie Wei , Xue-Feng Wu , En-Wei Liang

Using the sample of long Gamma-ray bursts (GRBs) detected by Swift-BAT before June 2007, we measure the cumulative distribution of the peak photon fluxes (log N - log P) of the Swift bursts. Compared with the BATSE sample, we find that the…

Astrophysics · Physics 2011-02-11 Xinyu Dai

We study the luminosity function (LF), the comoving rate and the detection rate of Long Gamma-Ray Burst (LGRBs) to high redshift, using galaxy catalogues constructed by combining high-resolution N-body simulations with semi-analytic models…

High Energy Astrophysical Phenomena · Physics 2015-05-19 M. A. Campisi , L. -X. Li , P. Jakobsson
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