Paper
15 July 2010 An apodizing phase plate coronagraph for VLT/NACO
Author Affiliations +
Abstract
We describe a coronagraphic optic for use with CONICA at the VLT that provides suppression of diffraction from 1.8 to 7 λ/D at 4.05 microns, an optimal wavelength for direct imaging of cool extrasolar planets. The optic is designed to provide 10 magnitudes of contrast at 0.2 arcseconds, over a "D" shaped region in the image plane, without the need for any focal plane occulting mask.
© (2010) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Matthew A. Kenworthy, Sascha P. Quanz, Michael R. Meyer, Markus E. Kasper, Rainer Lenzen, Johanan L. Codona, Julien H.V. Girard, and Philip M. Hinz "An apodizing phase plate coronagraph for VLT/NACO", Proc. SPIE 7735, Ground-based and Airborne Instrumentation for Astronomy III, 773532 (15 July 2010); https://doi.org/10.1117/12.856811
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CITATIONS
Cited by 17 scholarly publications.
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KEYWORDS
Point spread functions

Coronagraphy

Stars

Planets

Diffraction

Exoplanets

Telescopes

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