Gemini multiconjugate adaptive optics system review – II. Commissioning, operation and overall performance

Autor: Gelys Trancho, Cristian Moreno, Maxime Boccas, William Rambold, Ramon Galvez, Andrew Serio, Felipe Colazo, Gustavo Arriagada, Chadwick A. Trujillo, Matthieu Bec, Vanessa Montes, Vincent Garrel, Javier Luhrs, Francois Rigaut, Eduardo Marin, Benoit Neichel, Michelle L. Edwards, Vincent Fesquet, Sarah J. Diggs, Tomislav Vucina, Peter J. Young, Claudia Winge, Angelic Ebbers, Marcos A. van Dam, Peter Pessev, Celine d'Orgeville, Claudio Marchant, Fabrice Vidal, Eleazar R. Carrasco, Ariel Lopez, Peter J. McGregor, Cristian Urrutia, Gaston Gausachs
Přispěvatelé: Laboratoire d'Astrophysique de Marseille (LAM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Laboratoire Interdisciplinaire de Physique [Saint Martin d’Hères] (LIPhy), Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Fraser of Allander Institute, University of Strathclyde [Glasgow], Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)
Rok vydání: 2014
Předmět:
Zdroj: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2014, 440 (2), pp.1002--1019. ⟨10.1093/mnras/stu403⟩
Monthly Notices of the Royal Astronomical Society, 2014, 440 (2), pp.1002--1019. ⟨10.1093/mnras/stu403⟩
ISSN: 1365-2966
0035-8711
Popis: The Gemini Multi-conjugate Adaptive Optics System - GeMS, a facility instrument mounted on the Gemini South telescope, delivers a uniform, near diffraction limited images at near infrared wavelengths (0.95 microns- 2.5 microns) over a field of view of 120 arc seconds. GeMS is the first sodium layer based multi laser guide star adaptive optics system used in astronomy. It uses five laser guide stars distributed on a 60 arc seconds square constellation to measure for atmospheric distortions and two deformable mirrors to compensate for it. In this paper, the second devoted to describe the GeMS project, we present the commissioning, overall performance and operational scheme of GeMS. Performance of each sub-system is derived from the commissioning results. The typical image quality, expressed in full with half maximum, Strehl ratios and variations over the field delivered by the system are then described. A discussion of the main contributor to performance limitation is carried-out. Finally, overheads and future system upgrades are described.
20 pages, 11 figures, accepted for publication in MNRAS
Databáze: OpenAIRE