Recent progress on CCDs for astronomical imaging

被引：20

作者：

Groom, DE ^{[1
]}

机构：

[1] Univ Calif Berkeley, Lawrence Berkeley Lab, Berkeley, CA 94720 USA

来源：

OPTICAL AND IR TELESCOPE INSTRUMENTATION AND DETECTORS, PTS 1 AND 2 | 2000年 / 4008卷

关键词：

CCD; mosaic; high resistivity; fully depleted; PSF; astronomical; fringing; Lawrence Berkeley National Laboratory; Lick Observatory;

D O I：

10.1117/12.395522

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We review recent progress in the field, using as a framework a partial list of present limitations and problems: CCD and mosaic size, packing fraction in mosaics, red response and fringing, and intrinsic point-spread function due to lateral charge diffusion. Related topics such as orthogonal-transfer CCDs and the special requirements of adaptive-optics wavefront sensors are also discussed. Only cursory attention is given to other relevant issues, such as readout speed and anti-blooming techniques.

引用

页码：634 / 645

页数：12

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