Paper
11 July 2018 The segmented pupil experiment for exoplanet detection: Part 3. Advances and first light with segments cophasing
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Abstract
SPEED (Segmented Pupil Experiment for Exoplanet Detection) is an instrumental testbed designed to offer an ideal cocoon to provide relevant solutions in both cophasing and high-contrast imaging with segmented telescopes. The next generation of observatories will be made of a primary mirror with excessive complexity (mirror segmentation, central obscuration, and spider vanes) undoubtedly known to be unfavorable for the direct detection of exoplanets. Exoplanets detection around late-type stars (M-dwarfs) constitutes an outstanding reservoir of candidates, and SPEED integrates all the recipes to pave the road for this science case (cophasing sensors, multi-DM wavefront control and shaping architecture as well as advanced coronagraphy). In this paper, we provide a progress overview of the project and report on the first light with segments cophasing control and monitoring from a coronagraphic image.
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
P. Martinez, P. Janin-Potiron, M. Beaulieu, C. Gouvret, J. Dejonghe, A. Spang, M. Postnikova, P. Baudoz, O. Guyon, O. Preis, L. Abe, M. N'Diaye, and A. Marcotto "The segmented pupil experiment for exoplanet detection: Part 3. Advances and first light with segments cophasing", Proc. SPIE 10703, Adaptive Optics Systems VI, 1070357 (11 July 2018); https://doi.org/10.1117/12.2313551
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Cited by 1 scholarly publication.
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KEYWORDS
Image segmentation

Telescopes

Coronagraphy

Adaptive optics

Mirrors

Sensors

Space telescopes

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