Paper
14 February 2003 Polarimetry with adaptive optics at ESO Very Large Telescope (Yepun)
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Abstract
We present and discuss the capabilities of the infrared polarimetric modes of the ESO-VLT adaptive optics system NAOS-CONICA. Commissioning results obtained both with wire-grids and Wollaston prisms are shown. In particular, NACO observations of the Calabash reflection nebula are compared with earlier, seeing limited, results obtained at ESO to illustrate the new potential offered by adaptive optics assisted polarimetry on an 8m class telescope.
© (2003) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Nancy Ageorges, Rainer Lenzen, Markus Hartung, Wolfgang Brandner, Eric Gendron, Alan F. M. Moorwood, and Anne-Marie Lagrange "Polarimetry with adaptive optics at ESO Very Large Telescope (Yepun)", Proc. SPIE 4843, Polarimetry in Astronomy, (14 February 2003); https://doi.org/10.1117/12.459344
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Cited by 1 scholarly publication.
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KEYWORDS
Polarization

Polarimetry

Prisms

Adaptive optics

Telescopes

Calibration

Infrared radiation

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