Computation of the atmospheric dispersion effect on the Point Spread Function of a telescope and astronomical instrument

Development of python module for the computation of the Atmospheric Dispersion: the precise computation of the effect of the atmospheric dispersion requires the knowledge and simulation of the stellar spectrum and its convolution with the telescope and instrumental PSF. The goal would be the production of a general purpose python module able to produce an accurate and realistic dispersed PSF. With possible verification on-sky.