GeMS first on-sky results

François Rigaut*, Benoit Neichel, Maxime Boccas, Céline D'Orgeville, Gustavo Arriagada, Vincent Fesquet, Sarah J. Diggs, Claudio Marchand, Gaston Gausachs, William N. Rambold, Javier Lurhs, Shane Walker, Eleazar Rodrigo Carrasco-Damele, Michelle L. Edwards, Peter Pessev, Ramon L. Galvez, Tomislav B. Vucina, Claudio Araya, Alejandro Gutierrez, Angelic W. EbbersAndrew Serio, Cristian Moreno, Cristian Urrutia, Rolando Rogers, Roberto Rojas, Chadwick Trujillo, Brian Miller, Douglas A. Simons, Ariel Lopez, Vanesa Montes, Herman Diaz, Felipe Daruich, Felipe Colazo, Matthieu Bec, Gelys Trancho, Michael Sheehan, Peter McGregor, Peter J. Young, Matthew C. Doolan, Jan Van Harmelen, Brent L. Ellerbroek, Damien Gratadour, Aurea Garcia-Rissmann

*Corresponding author for this work

    Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

    46 Citations (Scopus)


    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.

    Original languageEnglish
    Title of host publicationAdaptive Optics Systems III
    Publication statusPublished - 2012
    EventAdaptive Optics Systems III - Amsterdam, Netherlands
    Duration: 1 Jul 20126 Jul 2012

    Publication series

    NameProceedings of SPIE - The International Society for Optical Engineering
    ISSN (Print)0277-786X


    ConferenceAdaptive Optics Systems III


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