scholarly journals LIFT: a focal-plane wavefront sensor for real-time low-order sensing on faint sources

2010 ◽  
Vol 35 (18) ◽  
pp. 3036 ◽  
Author(s):  
Serge Meimon ◽  
Thierry Fusco ◽  
Laurent M. Mugnier
2009 ◽  
Vol 509 ◽  
pp. A31 ◽  
Author(s):  
R. Galicher ◽  
P. Baudoz ◽  
G. Rousset ◽  
J. Totems ◽  
M. Mas

Author(s):  
B.R.M. Norris ◽  
J. Wei ◽  
C.H. Betters ◽  
A. Wong ◽  
S.G. Leon-Saval

2013 ◽  
Vol 8 (S299) ◽  
pp. 34-35 ◽  
Author(s):  
Thayne Currie ◽  
Olivier Guyon ◽  
Frantz Martinache ◽  
Christophe Clergeon ◽  
Michael McElwain ◽  
...  

AbstractWe present new on-sky results for the Subaru Coronagraphic Extreme Adaptive Optics imager (SCExAO) verifying and quantifying the contrast gain enabled by key components: the closed-loop coronagraphic low-order wavefront sensor (CLOWFS) and focal plane wavefront control (“speckle nulling”). SCExAO will soon be coupled with a high-order, Pyramid wavefront sensor which will yield > 90% Strehl ratio and enable 106–107 contrast at small angular separations allowing us to image gas giant planets at solar system scales. Upcoming instruments like VAMPIRES, FIRST, and CHARIS will expand SCExAO's science capabilities.


2020 ◽  
Vol 11 (1) ◽  
Author(s):  
Barnaby R. M. Norris ◽  
Jin Wei ◽  
Christopher H. Betters ◽  
Alison Wong ◽  
Sergio G. Leon-Saval

Abstract Adaptive optics (AO) is critical in astronomy, optical communications and remote sensing to deal with the rapid blurring caused by the Earth’s turbulent atmosphere. But current AO systems are limited by their wavefront sensors, which need to be in an optical plane non-common to the science image and are insensitive to certain wavefront-error modes. Here we present a wavefront sensor based on a photonic lantern fibre-mode-converter and deep learning, which can be placed at the same focal plane as the science image, and is optimal for single-mode fibre injection. By measuring the intensities of an array of single-mode outputs, both phase and amplitude information on the incident wavefront can be reconstructed. We demonstrate the concept with simulations and an experimental realisation wherein Zernike wavefront errors are recovered from focal-plane measurements to a precision of 5.1 × 10−3 π radians root-mean-squared-error.


2010 ◽  
Author(s):  
P. Baudoz ◽  
M. Mas ◽  
R. Galicher ◽  
G. Rousset

Author(s):  
Benjamin L. Gerard ◽  
Jean-Pierre Véran ◽  
Garima Singh ◽  
Glen Herriot ◽  
Olivier Lardière ◽  
...  

2016 ◽  
Vol 588 ◽  
pp. A136 ◽  
Author(s):  
J. R. Delorme ◽  
R. Galicher ◽  
P. Baudoz ◽  
G. Rousset ◽  
J. Mazoyer ◽  
...  

Author(s):  
Christian Marois ◽  
Benjamin L. Gerard ◽  
Olivier Lardière ◽  
Andre Anthony ◽  
Colin Bradley ◽  
...  

Author(s):  
Alex R. Cunha Lima ◽  
Arthur M. Medeiros ◽  
Vitor G. Marques ◽  
Manuel M. Oliveira

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