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An Imaging Polarimeter(IMPOL) for multi-wavelength observations

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arxiv astro-ph/9701028 v2 pith:4KYIKXDX submitted 1997-01-07 astro-ph

classification astro-ph
keywords polarizationanalyserdetectorimagingimpolobservationsparameterpolarimeter
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Taking advantage of the advances in array detector technology, an imaging polarimeter (IMPOL) has been constructed for measuring linear polarization in the wavelength band from 400-800 nm. It makes use of a Wollaston prism as the analyser to measure simultaneously the two orthogonal polarization components that define a Stoke's parameter. An achromatic half-wave plate is used to rotate the plane of polarization with respect to the axis of the analyser so that the second Stoke's parameter also can be determined. With a field of view correponding to about 30x30 sq. mm for a 1.2 m, f/13 telescope, a sensitive, liquid-nitrogen cooled CCD camera as the detector and a built-in acquisition and guidance unit, the instrument can be used for studying stellar fields or extended objects with an angular resolution close to 2 arcsec. The instrumental polarization is less than 0.05% and the accuracies of measurement are primarily limited by photon noise for typical observations.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 63 citations worldwide. Full citation record

  1. DHARA: Data Handling and Automated Reduction pipeline for AIMPOL

    astro-ph.IM 2026-07 accept novelty 6.0 of 10

    An automated Python pipeline for AIMPOL dual-beam polarimetry recovers literature polarization values within 2σ for standards and the Alessi 1 cluster and is adaptable to similar instruments.

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