Jean Pierre Veran, Henri-François Raynaud, Carlos Correia, Benoit Neichel, Guido Agapito, Gaetano Sivo, Fabrice Vidal, Olivier Guyon, Simone Esposito, Fernando Quiros-Pacheco, Lorenzo Pettazzi, Frantz Martinache, Jean Marc Conan, Richard Clare, Julian C. Christou, Caroline Kulcsár, Tim Morris, Eric Gendron, Andrés Guesalaga, Gérard Rousset, Enrico Fedrigo, Serge Meimon, Francois Rigaut, Riccardo Muradore, Laboratoire de Traitement et Transport de l'Information (L2TI), Université Paris 13 (UP13)-Institut Galilée-Université Sorbonne Paris Cité (USPC), ONERA - The French Aerospace Lab [Châtillon], ONERA-Université Paris Saclay (COmUE), Gemini Observatory, University of Hawai'i [Hilo], Universidad Católica de la Santísima Concepción (UCSC), NRC Herzberg Institute of Astrophysics, National Research Council of Canada (NRC), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA (UMR_8109)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Department of Physics [Durham University], Durham University, INAF - Osservatorio Astrofisico di Arcetri (OAA), Istituto Nazionale di Astrofisica (INAF), European Southern Observatory (ESO), Department of Computer Science [Verona] (UNIVR | DI), University of Verona (UNIVR), Subaru Telescope, National Astronomical Observatory of Japan (NAOJ), ONERA, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Dipartimento di Informatica [Verona], and Università degli Studi di Verona
We present in this paper an analysis of several tip-tilt on-sky data registered on adaptive optics systems installed on different telescopes (Gemini South, William Herschel Telescope, Large Binocular Telescope, Very Large Telescope, Subaru). Vibration peaks can be detected, and it is shown that their presence and location may vary, and that their origin is not always easy to determine. Mechanical solution that have been realized to mitigate vibrations are presented. Nevertheless, residual vibrations may still affect the instruments' performance, ranging from narrow high frequency vibration peaks to wide low frequency windshake-type perturbations. Power Spectral Densities (PSDs) of on-sky data are presented to evidence these features. When possible, indications are given regarding the gain in performance that could be achieved with adequate controllers accounting for vibration mitigation. Two examples of controller identification and design illustrate their ability to compensate for various types of disturbances (turbulence, windshake, vibration peaks, ...), showing a significant gain in performance. © 2012 SPIE., Adaptive Optics Systems III, July 1-6, 2012, Amsterdam, the Netherlands, Series: Proceedings of SPIE; no. 8447