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BASIS: Bayfordbury single-object integral field spectrograph

dc.contributor.authorRichards, S.
dc.contributor.authorMartin, Bill
dc.contributor.authorCampbell, D.
dc.contributor.authorJones, H.R.A.
dc.contributor.authorBland-Hawthorn, J.
dc.contributor.authorLawrence, J.
dc.contributor.authorBrinks, E.
dc.contributor.authorBryant, J.J.
dc.contributor.authorFogarty, L.
dc.contributor.authorGallaway, M.
dc.contributor.authorGoodwin, M.
dc.contributor.authorLeon-Saval, S.
dc.contributor.authorSarzi, M.
dc.contributor.authorSmith, Daniel
dc.contributor.editorMclean, Ian S.
dc.contributor.editorRamsay, Suzanne K.
dc.contributor.editorTakami, Hideki
dc.date.accessioned2014-03-10T09:29:05Z
dc.date.available2014-03-10T09:29:05Z
dc.date.issued2012-09
dc.identifier.citationRichards , S , Martin , B , Campbell , D , Jones , H R A , Bland-Hawthorn , J , Lawrence , J , Brinks , E , Bryant , J J , Fogarty , L , Gallaway , M , Goodwin , M , Leon-Saval , S , Sarzi , M & Smith , D 2012 , BASIS: Bayfordbury single-object integral field spectrograph . in I S Mclean , S K Ramsay & H Takami (eds) , Ground-based and Airborne Instrumentation for Astronomy IV . Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series , vol. 8446 , SPIE . https://doi.org/10.1117/12.925378
dc.identifier.otherPURE: 2826632
dc.identifier.otherPURE UUID: 9f9a3512-e761-4950-a939-47e4bb90a991
dc.identifier.otherBibtex: urn:40cb5d1df1c4a0ef45427dd9528e479d
dc.identifier.otherScopus: 84871955528
dc.identifier.otherORCID: /0000-0002-7758-9699/work/30407810
dc.identifier.otherORCID: /0000-0003-0757-6689/work/41936777
dc.identifier.otherORCID: /0000-0001-9708-253X/work/69424326
dc.identifier.urihttp://hdl.handle.net/2299/13046
dc.description.abstractWe present an inexpensive (<US$500) and easily replicable integral field unit for use on small aperture telescopes. Based on a commercial small spectrograph (SBIG Self-Guiding Spectrograph) and a 37 optical fibre bundle integral field unit with each fibre having 50μm cores and a pitch of 125μm. It has an overall field-of-view of 40 arc seconds (2.6arcsec/core), a resolution of 9Å from 3995Å to 7170Å and an average system efficiency of 9%, yielding a signal-tonoise ratio of 10 for a 20min exposure of a 13mag/arcsec2 source. Still in commissioning, we present first light observations of Vega and M57. © (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). [Downloading of the abstract is permitted for personal use only]en
dc.language.isoeng
dc.publisherSPIE
dc.relation.ispartofGround-based and Airborne Instrumentation for Astronomy IV
dc.relation.ispartofseriesSociety of Photo-Optical Instrumentation Engineers (SPIE) Conference Series
dc.titleBASIS: Bayfordbury single-object integral field spectrographen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Atmospheric and Climate Physics Research
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
rioxxterms.versionofrecordhttps://doi.org/10.1117/12.925378
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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