FN Archimer Export Format
PT C
TI The Phase-Shifted Zernike wave-front sensor
BT 
AF CISSE, Mahawa
   CHAMBOULEYRON, Vincent
   FAUVARQUE, Olivier
   BOND, Charlotte Z.
   LEVRAUD, Nicolas
   SAUVAGE, Jean -Francois
   NEICHEL, Benoit
   FUSCO, Thierry
AS 1:1,2;2:1;3:3;4:4;5:2,5;6:2;7:1;8:2;
FF 1:;2:;3:PDG-REM-RDT-LDCM;4:;5:;6:;7:;8:;
C1 Aix Marseille Univ., CNRS, CNES, Lab. d'Astrophysique de Marseille (France)
   DOTA, ONERA, Univ. Paris Saclay (France)
   IFREMER, Lab. Detection, Capteurs et Mesures (LDCM) (France)
   UK Astronomy Technology Ctr. (United Kingdom)
   INAF, Osservatorio Astrofisico di Arcetri (Italy)
C2 UNIV AIX MARSEILLE, FRANCE
   ONERA, FRANCE
   IFREMER, FRANCE
   UK ASTRON TECHNOL CTR, UK
   INAF OSSERV ASTROFIS ARCETRI, ITALY
SI BREST
SE PDG-REM-RDT-LDCM
IN WOS Ifremer UPR
   copubli-france
   copubli-europe
   copubli-univ-france
UR https://archimer.ifremer.fr/doc/00801/91283/100749.pdf
LA English
DT Proceedings paper
DE ;Giant telescopes;adaptive optics;wave-front sensor;high performance;data fusion
AB The next generation of Giant Fragmented Telescopes will allow the study of faint and distant objects such as exoplanets. But the structure of the telescope also brings new challenges such as pupil fragmentation or Low-Wind Effect (LWE) that needs to be corrected by the Adaptive Optics (AO) system. The Wave-Front Sensor (WFS) which is the heart of the AO system needs to be able to measure these aberrations. Because of its high sensitivity, the Zernike Wave-Front Sensor (ZWFS) appears to be a viable candidate as a 2nd stage instrument to measure telescope seeing or differential piston. However, its use is limited by its small dynamic range. We propose here a new concept of WFS based on the ZWFS with a better dynamic range : the Phase Shifted ZWFS (Phase-Shifted ZWFS).
PY 2022
CT Proceedings SPIE. Volume 12185, Adaptive Optics Systems VIII, 121850X (29 August 2022), 8p. + presentation
DI 10.1117/12.2628885
ID 91283
ER

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