主要内容:
用X-shooter,主要可以观测宿主星系的特性
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文章信息:
- · Electronic Refereed Journal Article (HTML)
- · Full Refereed Journal Article (PDF/Postscript)
- · arXiv e-print (arXiv:1108.1061)
- · References in the article
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Title: |
| Absorption spectroscopy of gamma-ray burst afterglows: Probing the GRB line of sight |
Authors: |
| D'Elia, V. |
Affiliation: |
| AA(ASI Science Data Centre, Via Galileo Galilei, 00044 Frascati (RM), Italy; INAF - Osservatorio Astronomico di Roma, Via di Frascati, 33, 00040 Monteporzio Catone, Italy) |
Publication: |
| Astronomische Nachrichten, Vol.332, Issue 3, p.272 (AN Homepage) |
Publication Date: |
| 03/2011 |
Origin: |
| AN |
Keywords: |
| gamma rays: bursts, ISM: abundances, ISM: kinematics and dynamics, ISM: structure, line: profiles |
Abstract Copyright: |
| (c) 2011: WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim |
DOI: |
| 10.1002/asna.201111533 |
Bibliographic Code: |
| 2011AN....332..272D |
Abstract
GRB absorption spectroscopy opened up a new window in the study of the high redshift Universe, especially with the launch of the Swift satellite and the quick and precise localization of the afterglow. Eight-meter class telescopes can be repointed within a few hours from the GRB, enabling the acquisition of high signal-to-noise ratio and high resolution afterglow spectra. In this paper I will give a short review of what we learned through this technique, and I will present some of the first results obtained with the X-shooter spectrograph.
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