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Proceedings Paper

Near-infrared aberration tracking using a correlation algorithm on the Galactic Center
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Paper Abstract

The GRAVITY acquisition camera has four 9x9 Shack-Hartmann sensors operating in the near-infrared. It measures the slow variations of a quasi-distorted wavefront of four telescope beams simultaneously, by imaging the Galactic Center field. The Shack-Hartmann lenslet images of the Galactic Center are generated. Since the lenslet array images are filled with the crowded Galactic Center stellar field, an extended object, the local shifts of the distorted wavefront have to be estimated with a correlation algorithm. In this paper we report on the accuracy of six existing centroid algorithms for the Galactic Center stellar field. We show the VLTI tunnel atmospheric turbulence phases are reconstructed back with a precision of 100 nm at 2 s integration.

Paper Details

Date Published: 21 July 2014
PDF: 11 pages
Proc. SPIE 9148, Adaptive Optics Systems IV, 91485B (21 July 2014); doi: 10.1117/12.2055869
Show Author Affiliations
Narsireddy Anugu, Univ. do Porto (Portugal)
Paulo Garcia, Univ. do Porto (Portugal)
Antonio Amorim, Univ. de Lisboa (Portugal)
Paulo Gordo, Univ. de Lisboa (Portugal)
Frank Eisenhauer, Max-Planck-Institut für extraterrestrische Physik (Germany)
Guy Perrin, Observatoire de Paris à Meudon, CNRS (France)
Wolfgang Brandner, Max-Planck-Institut für Astronomie (Germany)
Christian Straubmeier, Univ. zu Köln (Germany)
Karine Perraut, Institut de Planétologie et d’Astrophysique de Grenoble, CNRS (France)


Published in SPIE Proceedings Vol. 9148:
Adaptive Optics Systems IV
Enrico Marchetti; Laird M. Close; Jean-Pierre Véran, Editor(s)

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