activity
20092022
most citedThe CoRoT satellite in flight : description and performance

821 citations · 942 across the 10 of their papers we have counts for

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7 papers · 1 filter

astro-ph.IM2022★ 1 cited

Adapting the pyramid wavefront sensor for pupil fragmentation of the ELT class telescopes

Nicolas Levraud, Vincent Chambouleyron, Olivier Fauvarque +8

The next generation of Extremely Large Telescope (24 to 39m diameter) will suffer from the so-called "pupil fragmentation" problem. Due to their pupil shape complexity (segmentatio…

astro-ph.IM2021

Active deployable primary mirrors on CubeSat

Noah Schwartz, Maria Milanova, William Brzozowski +9

The volume available on small satellites restricts the size of optical apertures to a few centimetres, limiting the Ground-Sampling Distance (GSD) in the visible to typically 3 m a…

astro-ph.IM2020★ 37 cited

Pyramid wavefront sensor optical gains compensation using a convolutional model

Vincent Chambouleyron, Olivier Fauvarque, Pierre Janin-Potiron +5

Extremely Large Telescopes have overwhelmingly opted for the Pyramid wavefront sensor (PyWFS) over the more widely used Shack-Hartmann WaveFront Sensor (SHWFS) to perform their Sin…

astro-ph.IM2020

Design of the HARMONI Pyramid WFS module

Noah Schwartz, Jean-François Sauvage, Edgard Renault +12

Current designs for all three extremely large telescopes show the overwhelming adoption of the pyramid wavefront sensor (P-WFS) as the WFS of choice for adaptive optics (AO) system…

astro-ph.IM2018★ 9 cited

Laboratory Demonstration of an Active Optics System for High-Resolution Deployable CubeSat

Noah Schwartz, David Pearson, Stephen Todd +8

In this paper we present HighRes: a laboratory demonstration of a 3U CubeSat with a deployable primary mirror that has the potential of achieving high-resolution imaging for Earth…

astro-ph.IM2018★ 16 cited

Sensing and control of segmented mirrors with a pyramid wavefront sensor in the presence of spiders

Noah Schwartz, Jean-François Sauvage, Carlos Correia +9

The segmentation of the telescope pupil (by spiders & the segmented M4) create areas of phase isolated by the width of the spiders on the wavefront sensor (WFS), breaking the spati…

astro-ph.IM2018★ 22 cited

The adaptive optics modes for HARMONI: from Classical to Laser Assisted Tomographic AO

B. Neichel, T. Fusco, J. -F. Sauvage +25

HARMONI is a visible and NIR integral field spectrograph, providing the E-ELT's core spectroscopic capability at first light. HARMONI will work at the diffraction limit of the E-EL…