Can we use GRB to probe high redshift star formation?

F. Fiore; D. Guetta; S. Piranomonte; V. D'Elia; L. A. Antonelli

doi:10.1393/ncb/i2007-10267-0

Can we use GRB to probe high redshift star formation?

F. Fiore, D. Guetta, S. Piranomonte, V. D'Elia, L. A. Antonelli

Research output: Contribution to journal › Article › peer-review

Abstract

We present a detailed analysis of the selection effects that plague GRB observations. We find that these effects may partially explain the different redshift distributions between BeppoSax/HETE2 and Swift bursts. It is mandatory to consider these effects to determine the redshift evolution of GRBs.

Original language	English
Pages (from-to)	1395-1402
Number of pages	8
Journal	NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-GENERAL PHYSICS RELATIVITY ASTRONOMY AND MATHEMATICAL PHYSICS AND METHODS
Volume	121
Issue number	10-11
DOIs	https://doi.org/10.1393/ncb/i2007-10267-0
State	Published - 2006
Externally published	Yes

Access to Document

10.1393/ncb/i2007-10267-0

Cite this

@article{cabaa8b8526d4f0fae9d69b8e695c220,

title = "Can we use GRB to probe high redshift star formation?",

abstract = "We present a detailed analysis of the selection effects that plague GRB observations. We find that these effects may partially explain the different redshift distributions between BeppoSax/HETE2 and Swift bursts. It is mandatory to consider these effects to determine the redshift evolution of GRBs.",

author = "F. Fiore and D. Guetta and S. Piranomonte and V. D'Elia and Antonelli, \{L. A.\}",

year = "2006",

doi = "10.1393/ncb/i2007-10267-0",

language = "אנגלית",

volume = "121",

pages = "1395--1402",

journal = "NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-GENERAL PHYSICS RELATIVITY ASTRONOMY AND MATHEMATICAL PHYSICS AND METHODS",

issn = "1594-9982",