Computer Science – Performance
Scientific paper
Dec 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pasp..103.1314g&link_type=abstract
Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 103, Dec. 1991, p. 1314-1322.
Computer Science
Performance
30
Astronomical Polarimetry, Astronomical Spectroscopy, Spectrographs, Astronomical Observatories, Beam Splitters, Charge Coupled Devices, Performance Prediction, Telescopes
Scientific paper
A design for an optical spectropolarimeter consisting of a Pancharatnam half-wave plate and a modified Glan-Taylor polarizing beam splitter retrofitted to an existing astronomical spectrograph is described. The wave plate has a retardance of 180 +/-2 deg over the entire design wavelength range from 3200 A to 1.1 micron. The calcite polarizing beam splitter has a beam separation of one beam diameter, and a low length-to-width ratio of 1.035, making efficient use of the limited space available in most spectrographs. Cassegrain CCD spectrographs on the Mount Locke 2.7-m and Mount Palomar 5-in telescopes have been retrofitted with spectropolarimeters of the type described. The combination of these 'superachromatic' polarimeter parts with the high-efficiency CCD detectors now used in these and many other astronomical spectrographs should lead to a great expansion of spectropolarimetry in many branches of astronomical research.
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