Point spread function of hexagonally segmented telescopes by new symmetrical formulation
Point spread function of hexagonally segmented telescopes by new symmetrical formulation
复制标题
采用新对称公式的六边形分段望远镜的点扩散函数
DOI:
10.1093/mnras/sty3052
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发表时间:
2019
期刊:
影响因子:
--
通讯作者:
T. Sumi
中科院分区:
文献类型:
--
作者:
S. Itoh;T. Matsuo;H. Shibai;T. Sumi
A point spread function of hexagonally segmented telescopes is derived by a new symmetrical formulation. By introducing three variables on a pupil plane, the Fourier transform of pupil functions is derived by a 3D Fourier transform. The permutations of three variables correspond to those of a regular triangle’s vertices on the pupil plane. The resultant diffraction amplitude can be written as a product of two functions of the three variables; the functions correspond to the sinc function and Dirichlet kernel used in the basic theory of diffraction gratings. The new expression makes it clear that hexagonally segmented telescopes are equivalent to diffraction gratings in terms of mathematical formulae.