The third development consists of a mathematical technique for computing the polychromatic PSF from monochromatic aberrations (Ravikumar, Thibos, & Bradley, 2008). This allows us to extend the data of Thibos et al. The second development consist of mathematical techniques for computing aberrations at a smaller pupil from those collected at a larger pupil (Díaz, Fernández-Dorado, Pizarro, & Arasa, 2009 Mahajan, 2010 Schwiegerling, 2002). The first is the collection of wave front aberration data, for one wavelength and pupil diameter, from 200 best-corrected eyes of 100 young visually healthy observers (Thibos et al., 2002). Our approach is enabled by three recent developments.
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