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dc.contributor.authorDavis, C.J.
dc.contributor.authorChrysostomou, A.
dc.contributor.authorHough, J.
dc.date.accessioned2008-02-01T11:36:27Z
dc.date.available2008-02-01T11:36:27Z
dc.date.issued2005
dc.identifier.citationDavis , C J , Chrysostomou , A & Hough , J 2005 , Opportunities for Imaging and Spectro-Polarimetry at UKIRT . in In: Astronomical Polarimetry: Current Status and Future Directions - ASP Conference Series 343 . Astronomical Society of the Pacific , pp. 79-80 .
dc.identifier.isbn978-1-58381-277-8
dc.identifier.isbn1-58381-210-5
dc.identifier.otherdspace: 2299/1512
dc.identifier.urihttp://hdl.handle.net/2299/1512
dc.descriptionOriginal paper can be found at: http://161.58.115.79/pubs/cs/328.html--Copyright Astronomical Society of the Pacific
dc.description.abstractNear-IR imaging and spectro-polarimetry are offered with the facility instruments UIST and UFTI. Both linear and circular polarimetry are possible, the former from 1-5¹m, the latter from 1-2.5¹m. The IRPOL polarimetry module utilises Wollaston prisms (installed cold inside each instrument) and achromatic (JHK) or compound zero-order (LM) wave plates. Pipeline data reduction software is also available for all observing modes.en
dc.format.extent175805
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Astronomical Polarimetry: Current Status and Future Directions - ASP Conference Series 343
dc.titleOpportunities for Imaging and Spectro-Polarimetry at UKIRTen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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