A complete sample of long bright swift GRBs

G. Tagliaferri; R. Salvaterra; S. Campana; S. Covino; P. D'Avanzo; D. Fugazza; G. Ghirlanda; G. Ghisellini; A. Melandri; B. Sbarufatti; S. Vergani; L. Nava

doi:10.1051/eas/1361034

A complete sample of long bright swift GRBs

G. Tagliaferri, R. Salvaterra, S. Campana, S. Covino, P. D'Avanzo, D. Fugazza, G. Ghirlanda, G. Ghisellini, A. Melandri, B. Sbarufatti, S. Vergani, L. Nava

Astronomy & Astrophysics

Research output: Contribution to journal › Conference article › peer-review

Abstract

Starting from the Swift sample we defined a complete sub-sample of 58 bright long Gamma Ray Bursts (GRB), 52 of them (90%) with a redshift determination, in order to characterize their properties. This complete sample of bright long- GRBs allowed us to investigate their evolution with cosmic time and properties. We focused in particular on the GRB luminosity function, on the spectral-energy correlations of their prompt emission, on the nature of dark bursts and on possible correlations between the prompt and the X-ray afterglow properties.

Original language	English (US)
Pages (from-to)	229-233
Number of pages	5
Journal	EAS Publications Series
Volume	61
DOIs	https://doi.org/10.1051/eas/1361034
State	Published - 2013
Event	2012 Gamma-Ray Burst Symposium, GRB 2012 - Malaga, Spain Duration: Oct 8 2012 → Oct 12 2012

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
General Engineering
Space and Planetary Science

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10.1051/eas/1361034

Cite this

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title = "A complete sample of long bright swift GRBs",

abstract = "Starting from the Swift sample we defined a complete sub-sample of 58 bright long Gamma Ray Bursts (GRB), 52 of them (90%) with a redshift determination, in order to characterize their properties. This complete sample of bright long- GRBs allowed us to investigate their evolution with cosmic time and properties. We focused in particular on the GRB luminosity function, on the spectral-energy correlations of their prompt emission, on the nature of dark bursts and on possible correlations between the prompt and the X-ray afterglow properties.",

author = "G. Tagliaferri and R. Salvaterra and S. Campana and S. Covino and P. D'Avanzo and D. Fugazza and G. Ghirlanda and G. Ghisellini and A. Melandri and B. Sbarufatti and S. Vergani and L. Nava",

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doi = "10.1051/eas/1361034",

language = "English (US)",

volume = "61",

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TY - JOUR

T1 - A complete sample of long bright swift GRBs

AU - Tagliaferri, G.

AU - Salvaterra, R.

AU - Campana, S.

AU - Covino, S.

AU - D'Avanzo, P.

AU - Fugazza, D.

AU - Ghirlanda, G.

AU - Ghisellini, G.

AU - Melandri, A.

AU - Sbarufatti, B.

AU - Vergani, S.

AU - Nava, L.

PY - 2013

Y1 - 2013

N2 - Starting from the Swift sample we defined a complete sub-sample of 58 bright long Gamma Ray Bursts (GRB), 52 of them (90%) with a redshift determination, in order to characterize their properties. This complete sample of bright long- GRBs allowed us to investigate their evolution with cosmic time and properties. We focused in particular on the GRB luminosity function, on the spectral-energy correlations of their prompt emission, on the nature of dark bursts and on possible correlations between the prompt and the X-ray afterglow properties.

AB - Starting from the Swift sample we defined a complete sub-sample of 58 bright long Gamma Ray Bursts (GRB), 52 of them (90%) with a redshift determination, in order to characterize their properties. This complete sample of bright long- GRBs allowed us to investigate their evolution with cosmic time and properties. We focused in particular on the GRB luminosity function, on the spectral-energy correlations of their prompt emission, on the nature of dark bursts and on possible correlations between the prompt and the X-ray afterglow properties.

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U2 - 10.1051/eas/1361034

DO - 10.1051/eas/1361034

M3 - Conference article

AN - SCOPUS:84887044300

SN - 1633-4760

VL - 61

SP - 229

EP - 233

JO - EAS Publications Series

JF - EAS Publications Series

T2 - 2012 Gamma-Ray Burst Symposium, GRB 2012

Y2 - 8 October 2012 through 12 October 2012

ER -

A complete sample of long bright swift GRBs

Abstract

All Science Journal Classification (ASJC) codes

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