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Conference Paper: Wide-field multifiber spectroscopy with FLAIR II

TitleWide-field multifiber spectroscopy with FLAIR II
Authors
Editors
Editor(s):Crawford, DL
Issue Date1994
Citation
Instrumentation in Astronomy VIII, June 1, 1994, p. 65-74 How to Cite?
AbstractThe 1.2-m United Kingdom Schmidt Telescope has operated a wide- field spectroscopy service for a number of years. A new common- user system has recently been completed. The instrument, known as FLAIR II, offers many more fiber channels than its predecessors, together with wider spectral coverage and faster turn-round of target fields. This paper describes FLAIR II in its present-day form, highlighting the most innovative aspects of its design, and giving a critical evaluation of its performance. Its impact has been significant, and large data-sets are being accumulated for a variety of object-classes.
Persistent Identifierhttp://hdl.handle.net/10722/211221

 

DC FieldValueLanguage
dc.contributor.authorWatson, FG-
dc.contributor.authorParker, QA-
dc.contributor.authorCraine, ER-
dc.contributor.editorCrawford, DL-
dc.date.accessioned2015-07-08T03:23:16Z-
dc.date.available2015-07-08T03:23:16Z-
dc.date.issued1994-
dc.identifier.citationInstrumentation in Astronomy VIII, June 1, 1994, p. 65-74-
dc.identifier.urihttp://hdl.handle.net/10722/211221-
dc.description.abstractThe 1.2-m United Kingdom Schmidt Telescope has operated a wide- field spectroscopy service for a number of years. A new common- user system has recently been completed. The instrument, known as FLAIR II, offers many more fiber channels than its predecessors, together with wider spectral coverage and faster turn-round of target fields. This paper describes FLAIR II in its present-day form, highlighting the most innovative aspects of its design, and giving a critical evaluation of its performance. Its impact has been significant, and large data-sets are being accumulated for a variety of object-classes.-
dc.languageeng-
dc.relation.ispartofInstrumentation in Astronomy VIII-
dc.titleWide-field multifiber spectroscopy with FLAIR II-
dc.typeConference_Paper-
dc.identifier.emailParker, QA: quentinp@hku.hk-
dc.identifier.authorityParker, QA=rp02017-
dc.identifier.volume2198-
dc.identifier.spage65-
dc.identifier.epage74-

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