dc.contributor.author | Davis, C.J. | |
dc.contributor.author | Chrysostomou, A. | |
dc.contributor.author | Hough, J. | |
dc.date.accessioned | 2008-02-01T11:36:27Z | |
dc.date.available | 2008-02-01T11:36:27Z | |
dc.date.issued | 2005 | |
dc.identifier.citation | Davis , 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.isbn | 978-1-58381-277-8 | |
dc.identifier.isbn | 1-58381-210-5 | |
dc.identifier.other | dspace: 2299/1512 | |
dc.identifier.uri | http://hdl.handle.net/2299/1512 | |
dc.description | Original paper can be found at: http://161.58.115.79/pubs/cs/328.html--Copyright Astronomical Society of the Pacific | |
dc.description.abstract | Near-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.extent | 175805 | |
dc.language.iso | eng | |
dc.publisher | Astronomical Society of the Pacific | |
dc.relation.ispartof | In: Astronomical Polarimetry: Current Status and Future Directions - ASP Conference Series 343 | |
dc.title | Opportunities for Imaging and Spectro-Polarimetry at UKIRT | en |
dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
rioxxterms.type | Other | |
herts.preservation.rarelyaccessed | true | |