Swift gamma-ray burst Explorer: Afterglow follow-up and Swift constraints

Research output: Contribution to journalArticle

Abstract

The Swift mission has been conducting normal operations for approximately 15 months (since April 2005). During this time the mission has revolutionized the field of GRB afterglow follow-up - doubling the number of GRB afterglows with localization and adding a totally novel ability to study afterglows during the time between minutes to hours after the gamma-ray burst. I report on the efficiency of the Swift observatory for conducting these observations, and the science strategy of Swift operations, including fill-in targets and targets of opportunity.

Original languageEnglish (US)
Pages (from-to)1051-1054
Number of pages4
JournalNuovo Cimento della Societa Italiana di Fisica B
Volume121
Issue number10-11
DOIs
Publication statusPublished - Oct 1 2006

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All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)

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