The galaxy density environment of gamma-ray burst host galaxies
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 GRB host galaxies do not reside in high gal...
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2004
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Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v614_n1I_p84_Bornancini http://hdl.handle.net/20.500.12110/paper_0004637X_v614_n1I_p84_Bornancini |
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paper:paper_0004637X_v614_n1I_p84_Bornancini2023-06-08T14:28:49Z The galaxy density environment of gamma-ray burst host galaxies Cosmology: observations Gamma rays: bursts 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 GRB host galaxies do not reside in high galaxy density environments. Moreover, the host galaxy-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 Hubble Deep Field-North (HDF-N). 2004 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v614_n1I_p84_Bornancini http://hdl.handle.net/20.500.12110/paper_0004637X_v614_n1I_p84_Bornancini |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
Cosmology: observations Gamma rays: bursts |
spellingShingle |
Cosmology: observations Gamma rays: bursts The galaxy density environment of gamma-ray burst host galaxies |
topic_facet |
Cosmology: observations Gamma rays: bursts |
description |
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 GRB host galaxies do not reside in high galaxy density environments. Moreover, the host galaxy-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 Hubble Deep Field-North (HDF-N). |
title |
The galaxy density environment of gamma-ray burst host galaxies |
title_short |
The galaxy density environment of gamma-ray burst host galaxies |
title_full |
The galaxy density environment of gamma-ray burst host galaxies |
title_fullStr |
The galaxy density environment of gamma-ray burst host galaxies |
title_full_unstemmed |
The galaxy density environment of gamma-ray burst host galaxies |
title_sort |
galaxy density environment of gamma-ray burst host galaxies |
publishDate |
2004 |
url |
https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v614_n1I_p84_Bornancini http://hdl.handle.net/20.500.12110/paper_0004637X_v614_n1I_p84_Bornancini |
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1768543588948377600 |