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相关论文: Quantifying the Luminosity Evolution in Gamma-ray …

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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.…

天体物理学 · 物理学 2009-11-07 Nicole M. Lloyd-Ronning , Chris L. Fryer , Enrico Ramirez-Ruiz

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…

高能天体物理现象 · 物理学 2019-07-31 Guang-Xuan Lan , Hou-Dun Zeng , Jun-Jie Wei , Xue-Feng Wu

We derive, adopting a direct method, the luminosity function and the formation rate of long Gamma Ray Bursts through a complete, flux-limited, sample of Swift bursts which has a high level of completeness in redshift z (~82%). We…

高能天体物理现象 · 物理学 2016-02-17 A. Pescalli , G. Ghirlanda , R. Salvaterra , G. Ghisellini , S. D. Vergani , F. Nappo , O. S. Salafia , A. Melandri , S. Covino , D. Götz

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…

天体物理学 · 物理学 2015-05-13 R. Salvaterra , C. Guidorzi , S. Campana , G. Chincarini , G. Tagliaferri

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…

高能天体物理现象 · 物理学 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

Gamma Ray Bursts (GRBs) and galaxies at high redshift represent complementary probes of the star formation history of the Universe. In fact, both the GRB rate and the galaxy luminosity density are connected to the underlying star formation.…

宇宙学与河外天体物理 · 物理学 2015-06-16 M. Trenti , R. Perna , S. Tacchella

Gamma-ray bursts (GRBs) are powerful probes of the high-redshift universe. However, the proportion of collapsar GRBs among long GRBs and their event rate relative to the star formation rate (SFR) remain contentious issues. We assume that…

高能天体物理现象 · 物理学 2025-05-02 Yan-Kun Qu , Zhong-Xiao Man , Shuang-Xi Yi , Yu-Peng Yang

Gamma-ray bursts (GRBs) by virtue of their high luminosities can be detected up to very high redshifts and therefore can be excellent probes of the early universe. This task is hampered by the fact that most of their characteristics have a…

高能天体物理现象 · 物理学 2015-06-11 Vahe' Petrosian , Ellie Kitanidis , Daniel Kocevski

Evolution of the rate density of cosmological gamma-ray bursts (GRBs) is calculated and compared to the BATSE brightness distribution in the context of binary neutron-star mergers as the source of GRBs, taking account of the realistic star…

天体物理学 · 物理学 2010-04-06 Tomonori Totani

In this work, we restudy the dependence of luminosity function and event rates for different gamma-ray burst samples on the criteria of sample selection and threshold effect. To compare with many previous studies, we have chosen two samples…

高能天体物理现象 · 物理学 2022-04-20 X. F. Dong , X. J. Li , Z. B. Zhang , X. L. Zhang

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…

天体物理学 · 物理学 2009-10-31 Maarten Schmidt

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…

高能天体物理现象 · 物理学 2015-05-27 H. Yu , F. Y. Wang , Z. G. Dai , K. S. Cheng

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 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…

高能天体物理现象 · 物理学 2015-05-19 M. A. Campisi , L. -X. Li , P. Jakobsson

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…

高能天体物理现象 · 物理学 2022-06-15 G. Ghirlanda , R. Salvaterra

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…

天体物理学 · 物理学 2009-10-31 Maarten Schmidt

The source population of gamma-ray bursts (GRBs) declines towards the present epoch being consistent with the measured decline of the star formation rate. We show this using the brightness distribution of 3255 long BATSE GRBs found in an…

天体物理学 · 物理学 2009-11-07 B. E. Stern , Ya. Tikhomirova , R. Svensson

Gamma-ray Bursts (GRBs) are valuable probes of cosmic star formation reaching back into the epoch of reionization, and a large dataset with known redshifts ($z$) is an important ingredient for these studies. Usually, $z$ is measured using…

Long gamma-ray bursts (LGRBs) are typically thought to result from the collapse of massive stars. Nonetheless, recent observations of gamma-ray bursts (GRBs) 211211A and 230307A, coupled with the low-redshift excess of LGRB event rates…

高能天体物理现象 · 物理学 2025-05-12 Yan-Kun Qu , Zhong-Xiao Man , Zhi-Bin Zhang

Using the luminosity function and the apparent GRB rate inferred from the spectral peak energy-luminosity relation, we investigate the absolute GRB formation rate, taking into account the effects of both the jet-luminosity evolution and the…

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