Analysis of off-axis point spread function of astronomical adaptive systems for the site of San Pedro Martir
Por:
Orlov V.G., VOYTSEKHOVICH, VALERY, Sanchez L.J., Cuevas S., Avila R.
Publicada:
1 ene 2000
Resumen:
A detailed analysis of anisotropy in the point spread function (PSF) associated with off-axis adaptive astronomical correction is presented. The results obtained are based on the experimental Cn 2 profile which has been recently measured at San Pedro Martir observatory (Mexico). It is found that the PSF has a complicated shape that depends strongly on the wavelength and on the separation between the guide and observed stars.
Filiaciones:
Orlov V.G.:
Inst de Astronomia - UNAM, Mexico, Mexico
Sanchez L.J.:
Inst de Astronomia - UNAM, Mexico, Mexico
Cuevas S.:
Inst de Astronomia - UNAM, Mexico, Mexico
Avila R.:
Inst de Astronomia - UNAM, Mexico, Mexico
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