Wave-front sensor, as the main component of Adaptive optics system, detects light from the astronomic object or
reference sources. It aims to improve the utilization of light, especially for AO system work with the faint objects.
Compared with Shack-Hartmann sensor, pyramid wave-front sensor is a relatively new one with increased pupil
sampling and spatial resolution. Pyramid wave-front sensor uses a refractive element (the pyramid) to produce four
images of the entrance pupil. Usually, Single pyramid prototypes are made using the classical figuring and polishing
techniques. This approach, however, is not only very time consuming but also does not guarantee a uniform repeatability
of the optical characteristics of the pyramids. The loss of low frequency component increases due to the roofs existing on
its vertexes. Moreover, stray light is introduced in the four images. We therefore are investigating a modified pyramidal
optical components based on the binary optical concept. In this article we describe the diffractive pyramid prototypes
using the micro fabrication technique. The parameters of the pyramid are discussed.
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