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.
Original language | English |
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Title of host publication | In: Astronomical Polarimetry: Current Status and Future Directions - ASP Conference Series 343 |
Publisher | Astronomical Society of the Pacific |
Pages | 79-80 |
ISBN (Print) | 978-1-58381-277-8, 1-58381-210-5 |
Publication status | Published - 2005 |