Hostname: page-component-7bb8b95d7b-dtkg6 Total loading time: 0 Render date: 2024-09-29T17:12:42.448Z Has data issue: false hasContentIssue false
  • English
  • Français

Absorption features in the X-shooter GRB afterglow sample

Published online by Cambridge University Press:  27 October 2016

Antonio de Ugarte Postigo  and
for the X-shooter GRB collaboration
Antonio de Ugarte Postigo
Affiliation:
Instituto de Astrofísica de Andalucía (IAA-CSIC), Granada, Spain email: [email protected] Dark Cosmology Centre, NBI, U. Copenhagen, Copenhagen Ø, Denmark
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Since 2009 X-shooter has collected spectroscopy of over 80 gamma-ray burst afterglows with redshifts ranging from 0.05 to 6.3. Thanks to its efficiency, broad wavelength coverage (3,000 to 24,800 Å), and intermediate spectral resolution (R~8,000) it has become the most efficient tool for gamma-ray burst afterglow spectroscopy. In this Focus Meeting we presented the sample and some preliminary results of the analysis of absorption systems.

Keywords

gamma-rays: burstsastronomical data bases: miscellaneous
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29B: Astronomy in Focus , August 2015 , pp. 252
Copyright
Copyright © International Astronomical Union 2016 

References

de Ugarte Postigo, A. et al. 2012, A&A, 548, 11 Google Scholar
de Ugarte Postigo, A. et al. 2014, SPIE, 9152, 0 Google Scholar
Vernet, J., et al. 2011, A&A, 536, 105 Google Scholar