伽玛暴(Gamma-Ray Burst)笔记。记录有关伽玛暴的新文章,另外也包括看的老文章、自己的想法、以及跟天文相关的一些东西。 Feel free to leave me a message by comments or by email.

星期五, 八月 05, 2011

D'Elia 2011 余辉的谱观测

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:

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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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