EPJ Web of Conferences
Volume 16, 2011Research, Science and Technology of Brown Dwarfs and Exoplanets: Proceedings of an International Conference held in Shangai on Occasion of a Total Eclipse of the Sun
|Number of page(s)||2|
|Published online||18 July 2011|
XAO coronagraphy with the High-Order Test bench
European Southern Observatory, Karl-Schwarzschild-Strasse 2, 85748 Garching, Germany
a e-mail: firstname.lastname@example.org
Extreme adaptive optics systems dedicated to the search for extra solar planets are currently being developed for 8–10 meter class telescopes. The High-Order Test bench (HOT) is a high-contrast imaging adaptive optics bench developed at ESO. Its objective is to test and optimize different techniques and technologies (e.g. wave front sensors, coronagraphs, speckle calibration methods…). It mimics realistic conditions at a telescope (e.g. VLT), including turbulence generator, XAO, and various near-IR coronagraphs. Here we provide a short overview of the system, and present results of recent AO-closed loop coronagraphic runs obtained with an Apodized Pupil Lyot Coronagraph (APLC).
© Owned by the authors, published by EDP Sciences, 2011
Initial download of the metrics may take a while.