Efficiency of low-order adaptive correction for the San Pedro Mártir observatory: Experimental Results

Details Efficiency of low-order adaptive correction for the San Pedro Mártir observatory: Experimental Results Efficiency of low-order adaptive correction for the San Pedro Mártir observatory: Experimental Results

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..19...59v&link_type=abstract

San Pedro Mártir: Astronomical Site Evaluation (Eds. Irene Cruz-González, Remy Avila & Mauricio Tapia) Revista Mexicana de Astro

Physics

Optics

Atmospheric Effects, Instrumentation: Adaptive Optics, Turbulence

Scientific paper

The efficiency of low-order adaptive astronomical systems is estimated on the basis of experimental data obtained at San Pedro Martir observatory with dynamic Hartmann test. The estimation is performed for the 1.5 m telescope. The results show that for the V-band the low-order adaptive correction provides a good improvement in observed images, while for the K-band even the simplest tip/tilt correction gives a very noticeable improvement in the image quality.

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