Opportunities for Imaging and Spectro-Polarimetry at UKIRT

Details Opportunities for Imaging and Spectro-Polarimetry at UKIRT Opportunities for Imaging and Spectro-Polarimetry at UKIRT

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..343...79d&link_type=abstract

Astronomical Polarimetry: Current Status and Future Directions ASP Conference Series, Vol. 343, Proceedings of the Conference he

Astronomy and Astrophysics

Astronomy

1

Scientific paper

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 1-5μm, the latter from 1-2.5μm. 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.

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