Hostname: page-component-586b7cd67f-2plfb Total loading time: 0 Render date: 2024-11-23T11:30:20.806Z Has data issue: false hasContentIssue false

Absorption features in the X-shooter GRB afterglow sample

Published online by Cambridge University Press:  27 October 2016

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.

Type
Contributed Papers
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