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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…

天体物理学 · 物理学 2009-11-11 R. Salvaterra , C. Chincarini

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…

The accumulation of {\it Swift} observed gamma-ray bursts (GRBs) gradually makes it possible to directly derive a GRB luminosity function (LF) from observational luminosity distribution, where however two complexities must be involved as…

高能天体物理现象 · 物理学 2012-07-11 Xiao-Feng Cao , Yun-Wei Yu , K. S. Cheng , Xiao-Ping Zheng

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

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 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,…

In this work, we update and enlarge the long gamma-ray burst (GRB) sample detected by the {\it Swift} satellite. Given the incomplete sampling of the faint bursts and the low completeness in redshift measurement, we carefully select a…

高能天体物理现象 · 物理学 2021-09-15 Guang-Xuan Lan , Jun-Jie Wei , Hou-Dun Zeng , Ye Li , Xue-Feng Wu

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…

高能天体物理现象 · 物理学 2013-10-17 Wei-Wei Tan , Xiao-Feng Cao , Yun-Wei Yu

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

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 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…

高能天体物理现象 · 物理学 2015-10-14 W. W. Tan , F. Y. Wang

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

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

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 estimate the luminosity evolution and formation rate for over 900 GRBs by using redshift and luminosity data calculated by Band, Norris, $&$ Bonnell (2004) via the lag-luminosity correlation. By applying maximum likelihood techniques, we…

天体物理学 · 物理学 2009-11-11 Daniel Kocevski , Edison Liang

As of December 2023, the Swift satellite has detected more than 1600 gamma-ray bursts (GRBs). We select 307 Type II GRBs for constructing the luminosity function (LF) based on the following criteria: (1) duration $T_{90} \geq 2 s$; (2)…

高能天体物理现象 · 物理学 2025-05-19 Yan-Kun Qu , Zhong-Xiao Man , Yu-Peng Yang , Shuang-Xi Yi , Mei Du , Fa-yin Wang

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

We compute the probability to detect long Gamma Ray Bursts (GRBs) at z>5 with Swift, assuming that GRBs form preferentially in low-metallicity environments. The model fits well both the observed BATSE and Swift GRB differential peak flux…

天体物理学 · 物理学 2009-11-13 R. Salvaterra , S. Campana , G. Chincarini , G. Tagliaferri , S. Covino

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

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
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