LRIS imaging spectropolarimeter at the W.M. Keck Observatory

Details LRIS imaging spectropolarimeter at the W.M. Keck Observatory LRIS imaging spectropolarimeter at the W.M. Keck Observatory

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003spie.4843..146g&link_type=abstract

Polarimetry in Astronomy. Edited by Silvano Fineschi . Proceedings of the SPIE, Volume 4843, pp. 146-155 (2003).

Astronomy and Astrophysics

Astronomy

5

Scientific paper

An optical-wavelength polarimetry module has been in use for the past ten years at the W.M. Keck Observatory. The module is used in conjunction with the LRIS imaging spectrograph. It provides either imaging polarimetry or spectropolarimetry across the full wavelength range of the instrument (320-1100 nm). The design, performance, and limitations of the polarimetry module are described, along with a sampling of science results.

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