The vector vortex is a coronagraphic imaging mode of the recently commissioned Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) platform on the 8 m Subaru Telescope. This multi-purpose high-contrast visible and near-infrared (R- to K-band) instrument is not only intended to serve as a VLT-class "planet-imager" instrument in the northern...
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2018 (v1)Journal articleUploaded on: December 4, 2022
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September 2021 (v1)Journal article
Context. One of the key noise sources that currently limits high-contrast imaging observations for exoplanet detection is quasi-static speckles. Quasi-static speckles originate from slowly evolving non-common path aberrations (NCPA). These NCPA are related to the different optics encountered in the wavefront sensing path and the science path,...
Uploaded on: December 3, 2022 -
February 2021 (v1)Journal article
Context. One of the key challenges facing direct exoplanet imaging is the continuous maintenance of the region of high contrast within which light from the exoplanet can be detected above the stellar noise. In high-contrast imaging systems, the dominant source of aberrations is the residual wavefront error that arises due to non-common path...
Uploaded on: December 3, 2022 -
August 2017 (v1)Journal article
Photonic technologies offer numerous advantages for astronomical instruments such as spectrographs and interferometers owing totheir small footprints and diverse range of functionalities. Operating at the diffraction-limit, it is notoriously difficult to efficientlycouple such devices directly with large telescopes. We demonstrate that with...
Uploaded on: December 3, 2022 -
2013 (v1)Journal article
International audience
Uploaded on: December 2, 2022