Abstract: The AOtools package offers generic adaptive optics processing tools in addition to astronomy-specific methods; among these are analyzing data in the pupil plane, images and point spread functions in the focal plane, wavefront sensors, modeling of atmospheric turbulence, physical optical propagation of wavefronts, and conversion functions to convert stellar brightness into photon flux for a given waveband. The software also calculates integrated atmospheric parameters, such as coherence time and isoplanatic angle from atmospheric turbulence and wind speed profile.
Credit: Townson, M. J.; Farley, O. J. D.; Orban de Xivry, G.; Osborn, J.; Reeves, A. P.
Preferred citation method: https://ui.adsabs.harvard.edu/abs/2019OExpr..2731316T
Reason: Updated code entry.