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The Astrophysical Journal
Article . 2004 . Peer-reviewed
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arXiv.org e-Print Archive
Preprint . 2004
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https://dx.doi.org/10.48550/ar...
Article . 2004
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Pontificia Universidad Católica de Chile: Repositorio UC
Article . 2017
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The Galaxy Density Environment of Gamma‐Ray Burst Host Galaxies

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 10 Oct 2004Embargo end date: 01 Jan 2004 English Publisher:American Astronomical SocietyJournal:The Astrophysical Journal, volume 614, pages 84-90 (issn: 0004-637X, eissn: 1538-4357, Copyright policy )
Authors: Bornancini, Carlos G.; Martinez, Hector J.; Lambas, Diego G.; Floc'h, Emeric Le; Mirabel, I. Felix; Minniti, Dante;

doi: 10.1086/392497 , 10.48550/arxiv.astro-ph/0402576

arXiv: astro-ph/0402576

The Galaxy Density Environment of Gamma‐Ray Burst Host Galaxies

Abstract

We analyze cross-correlation functions between Gamma-Ray Burst (GRB) hosts and surrounding galaxies. We have used data obtained with the Very Large Telescope at Cerro Paranal (Chile), as well as public Hubble Space Telescope data. Our results indicate that Gamma-Ray Burst host galaxies do not reside in high galaxy density environments. Moreover, the host-galaxy cross-correlations show a relatively low amplitude. Our results are in agreement with the cross-correlation function between star-forming galaxies and surrounding objects in the HDF-N.

6 figures, accepted for publication in ApJ

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Keywords

Astronomía, Galaxias, Astronomía - Observaciones, Astrophysics (astro-ph), FOS: Physical sciences, Rayos gamma, Astrophysics, 520

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
15
Average
Average
Top 10%
Green
gold
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