Poster + Paper
29 August 2022 A visible-light Lyot coronagraph for SCExAO/VAMPIRES
Miles Lucas, Michael Bottom, Olivier Guyon, Julien Lozi, Barnaby Norris, Vincent Deo, Sébastien Vievard, Kyohoon Ahn, Nour Skaf, Peter Tuthill
Author Affiliations +
Conference Poster
Abstract
We describe the design and initial results from a visible-light Lyot coronagraph for SCExAO/VAMPIRES. The coronagraph is comprised of four hard-edged, partially transmissive focal plane masks with inner working angles of 36 mas, 55 mas, 92 mas and 129 mas, respectively. The Lyot stop is a reflective, undersized design with a geometric throughput of 65.7%. Our preliminary on-sky contrast is 10−2 at 0.1 ′′ to 10−4 at 0.75′′ for all mask sizes. The coronagraph was deployed in early 2022 and is available for open use.
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Miles Lucas, Michael Bottom, Olivier Guyon, Julien Lozi, Barnaby Norris, Vincent Deo, Sébastien Vievard, Kyohoon Ahn, Nour Skaf, and Peter Tuthill "A visible-light Lyot coronagraph for SCExAO/VAMPIRES", Proc. SPIE 12184, Ground-based and Airborne Instrumentation for Astronomy IX, 121844E (29 August 2022); https://doi.org/10.1117/12.2632269
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KEYWORDS
Coronagraphy

Point spread functions

Satellites

Wavefronts

Calibration

Exoplanets

Photometry

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