Cordier 2008 中法卫星SVOM-如何更好地定红移

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Title:		SVOM pointing strategy: how to optimize the redshift measurements?
Authors:		Cordier, B.; Desclaux, F.; Foliard, J.; Schanne, S.
Affiliation:		AA(), AB(), AC(), AD()
Publication:		GAMMA-RAY BURSTS 2007: Proceedings of the Santa Fe Conference. AIP Conference Proceedings, Volume 1000, pp. 585-588 (2008). (AIPC Homepage)
Publication Date:		05/2008
Origin:		AIP
Keywords:		gamma-ray sources (astronomical), red shift, telescopes
Abstract Copyright:		(c) 2008: American Institute of Physics
DOI:		10.1063/1.2943538
Bibliographic Code:		2008AIPC.1000..585C

Abstract

The Sino-French SVOM mission (Space-based multi-band astronomical Variable Objects Monitor) has been designed to detect all known types of gamma-ray bursts (GRBs) and to provide fast and reliable GRB positions. In this study we present the SVOM pointing strategy which should ensure the largest number of localized bursts allowing a redshift measurement. The redshift measurement can only be performed by large telescopes located on Earth. The best scientific return will be achieved if we are able to combine constraints from both space segment (platform and payload) and ground telescopes (visibility).

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