Sensor Distortion Effects in Photon Monte Carlo Simulations

被引:4
|
作者
Peterson, J. R. [1 ]
O'Connor, P. [2 ]
Nomerotski, A. [2 ]
Magnier, E. [3 ]
Jernigan, J. G. [4 ]
Cheng, J. [1 ]
Cui, W. [1 ,5 ]
Peng, E. [1 ]
Rasmussen, A. [6 ]
Sembroski, G. [1 ]
机构
[1] Purdue Univ, Dept Phys & Astron, W Lafayette, IN 47907 USA
[2] Brookhaven Natl Lab, Upton, NY 11973 USA
[3] Univ Hawaii, Dept Astron, Honolulu, HI 96822 USA
[4] Eureka Sci, Oakland, CA 94602 USA
[5] Tsinghua Univ, Tsinghua Ctr Astrophys, Dept Astron, Beijing 100084, Peoples R China
[6] Stanford Linear Accelerator Lab, Menlo Pk, CA 94025 USA
来源
ASTROPHYSICAL JOURNAL | 2020年 / 889卷 / 02期
关键词
D O I
10.3847/1538-4357/ab64e0
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a detailed method to simulating sensor distortions using a photon and electron Monte Carlo method. We use three-dimensional electrostatic simulations to parameterize the perturbed electric field profile for nonideal sensor details. We follow the conversion of simulated photons, and the subsequent response of the converted electrons to the electric field pattern. These nonideal sensor details can be implemented efficiently in a Monte Carlo approach. We demonstrate that the nonideal sensor distortions have a variety of observable consequence including the modification of the astrometric pattern; the distortion of the electron diffusion size and shape; and the distortion of flats. We show analytic validation of the diffusion physics, reproduce two kinds of edge distortion, and show qualitative validation of field-free regions, lithography errors, and fringing. We also demonstrate that there are two related effects of doping variation having different observable consequences. We show that field distortions from accumulated electrons lead to intensity-dependent point-spread functions and the sublinear variance in flats. The method is implemented in the Photon Simulator and the code is publicly available.
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页数:12
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