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Concepts for a high-resolution multi-object spectrograph for galactic archeology on the Anglo-Australian Telescope

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Barden, Samuel Charles; Bland-Hawthorn, Joss; Churilov, Vladimir; Ellis, S; Farrell, Tony; Freeman, Kenneth; Haynes, Roger; Horton, Anthony; Jones, Damian; Knight, Greg; Miziarski, Stan

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Mapping out stellar families to trace the evolutionary star formation history of the Milky Way requires a spectroscopic facility able to deliver high spectral resolution (R 30k) with both good wavelength coverage (~400 Ang) and target multiplex advantage

dc.contributor.authorBarden, Samuel Charles
dc.contributor.authorBland-Hawthorn, Joss
dc.contributor.authorChurilov, Vladimir
dc.contributor.authorEllis, S
dc.contributor.authorFarrell, Tony
dc.contributor.authorFreeman, Kenneth
dc.contributor.authorHaynes, Roger
dc.contributor.authorHorton, Anthony
dc.contributor.authorJones, Damian
dc.contributor.authorKnight, Greg
dc.contributor.authorMiziarski, Stan
dc.coverage.spatialMarseille, France
dc.date.accessioned2015-12-08T22:40:05Z
dc.date.created23-28 June 2008
dc.identifier.isbn9780819472243
dc.identifier.urihttp://hdl.handle.net/1885/36348
dc.description.abstractMapping out stellar families to trace the evolutionary star formation history of the Milky Way requires a spectroscopic facility able to deliver high spectral resolution (R 30k) with both good wavelength coverage (~400 Ang) and target multiplex advantage
dc.publisherSPIE - The International Society for Optical Engineering
dc.relation.ispartofseriesGround-Based and Airborne Instrumentation for Astronomy II
dc.sourceGround-Based and Airborne Instrumentation for Astronomy II
dc.subjectKeywords: Anamorphic collimator; Anglo-australian observatories; Aperture telescope; Dispersion modes; Double pass; Echelle; High resolution; High spectral resolution; Milky ways; Multi-object; Multi-object spectrograph; Star formations; VPH gratings; Wavelength co Echelle; High resolution; Multi-object; Spectrograph; White pupil
dc.titleConcepts for a high-resolution multi-object spectrograph for galactic archeology on the Anglo-Australian Telescope
dc.typeConference paper
local.description.notesImported from ARIES
local.description.refereedNo
dc.date.issued2008
local.identifier.absfor020104 - Galactic Astronomy
local.identifier.ariespublicationu4362859xPUB135
local.type.statusPublished Version
local.contributor.affiliationBarden, Samuel Charles, Anglo-Australian Observatory
local.contributor.affiliationBland-Hawthorn, Joss, University of Sydney
local.contributor.affiliationChurilov, Vladimir, Anglo-Australian Observatory
local.contributor.affiliationEllis, S, Anglo-Australian Observatory
local.contributor.affiliationFarrell, Tony, Anglo-Australian Observatory
local.contributor.affiliationFreeman, Kenneth, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationHaynes, Roger, Anglo-Australian Observatory
local.contributor.affiliationHorton, Anthony, Anglo-Australian Observatory
local.contributor.affiliationJones, Damian, Prime Optics (Australia)
local.contributor.affiliationKnight, Greg, Sinclair Knight Merz
local.contributor.affiliationMiziarski, Stan, Anglo-Australian Observatory
local.description.embargo2037-12-31
local.bibliographicCitation.startpage1
local.bibliographicCitation.lastpage12
local.identifier.doi10.1117/12.788549
dc.date.updated2016-02-24T11:06:02Z
local.identifier.scopusID2-s2.0-66249104699
CollectionsANU Research Publications

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