Performance of the ESO AO system, Adonis, at La Silla 3.6 M telescope

Details Performance of the ESO AO system, Adonis, at La Silla 3.6 M telescope Performance of the ESO AO system, Adonis, at La Silla 3.6 M telescope

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997spie.3136..589b&link_type=abstract

Conference Paper, SPIE Proceedings, Vol. 3126, p. 589-594.

Physics

Optics

1

Adaptive Optics, Telescopes, Performance Tests, Calibrating, Performance Prediction, Reference Stars, Servocontrol

Scientific paper

We report on the calibration and field test results obtained with the ESO/Meudon Adaptive Optics System, Adonis. This 7x7, 50-cm subaperture system is now routinely in use at the ESO La Silla 3.6-m telescope, offered to astronomers together with two IR cameras covering the 1-5-micron wavelength range. The calibration activity summarized here has investigated the field performances achieved so far with natural guide stars using either the Reticon or the EBCCD wavefront sensors.

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