GeMS: first on-sky results
Author(s) -
F. Rigaut,
Benoît Neichel,
Maxime Boccas,
Céline d’Orgeville,
Gustavo Arriagada,
Vincent Fesquet,
Sarah J. Diggs,
Claudio Marchant,
Gaston Gausach,
William Rambold,
Javier Lührs,
Shane Walker,
Eleazar R. Carrasco-Damele,
Michelle L. Edwards,
Peter Pessev,
Ramon Galvez,
Tomislav Vučina,
Claudio Araya,
Alejandro Gutiérrez,
Angelic Ebbers,
Andrew Serio,
Cristian Moreno,
Cristian Urrutia,
Rolando Rogers,
Roberto G. Rojas,
Chadwick A. Trujillo,
Bryan W. Miller,
D. A. Simons,
Ariel Lopez,
Vanessa Montes,
Herman Diaz,
Felipe Daruich,
Felipe Colazo,
Matthieu Bec,
Gelys Trancho,
Michael P. Sheehan,
Peter McGregor,
P. Young,
Matthew Doolan,
Jan van Harmelen,
Brent L. Ellerbroek,
Damien Gratadour,
A. Garcia-Rissmann
Publication year - 2012
Publication title -
proceedings of spie, the international society for optical engineering/proceedings of spie
Language(s) - English
Resource type - Conference proceedings
SCImago Journal Rank - 0.192
H-Index - 176
eISSN - 1996-756X
pISSN - 0277-786X
DOI - 10.1117/12.927061
Subject(s) - strehl ratio , adaptive optics , centroid , sky , computer science , laser guide star , path (computing) , remote sensing , artificial intelligence , optics , physics , astronomy , geology , programming language
GeMS, the Gemini Laser Guide Star Multi-Conjugate Adaptive Optics facility system, has seen first light in December 2011, and has already produced images with H band Strehl ratio in excess of 35% over fields of view of 85x85 arcsec, fulfilling the MCAO promise. In this paper, we report on these early results, analyze trends in performance, and concentrate on key or novel aspects of the system, like centroid gain estimation, on-sky non common path aberration estimation. We also present the first astrometric analysis, showing very encouraging results.
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