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A 4-Megapixel Cooled CCD Division of Focal Plane Polarimeter for Celestial Imaging

机译:用于天体成像的焦平面旋光仪的4兆像素冷却CCD分区

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摘要

The field of astronomy relies on spectral and polarization imagery recorded across a wide range of spectra to make inferences about imaged objects from nearby and distant galaxies. One of the challenges in recording celestial polarization information is recording multiple images filtered with various polarization optics, such as linear polarization filters or retarders, and with low-noise, low-dark-current sensors. In this paper, we present a division of focal plane polarimeter that can operate at room temperature down to −20 °C. When the imaging sensor operates at −20 °C, the dark currents is reduced by two orders of magnitude, which improves the polarization extinction ratio by ~5-fold. Comprehensive optoelectronic tests are presented with data recorded with the polarimeter.
机译:天文学领域依赖于记录在广泛光谱范围内的光谱和极化图像,以推断来自附近星系和遥远星系的成像物体。记录天极化信息的挑战之一是记录用各种极化光学器件(例如线性极化滤波器或延迟器)以及低噪声,低暗电流传感器过滤的多个图像。在本文中,我们介绍了焦平面旋光计的一种划分方法,它可以在低至-20°C的室温下工作。当成像传感器在-20°C下工作时,暗电流减小了两个数量级,这将偏振消光比提高了约5倍。随偏振计记录的数据一起进行了全面的光电测试。

著录项

  • 来源
    《Sensors Journal, IEEE》 |2017年第9期|2725-2733|共9页
  • 作者单位

    Department of Computer Science and Engineering, Washington University in St. Louis, St. Louis, MO, USA;

    Department of Electrical and Systems Engineering, Washington University in St. Louis, St. Louis, MO, USA;

    Department of Computer Science and Engineering, Washington University in St. Louis, St. Louis, MO, USA;

    Department of Computer Science and Engineering, Washington University in St. Louis, St. Louis, MO, USA;

    Department of Electrical and Computer Engineering, University of Illinois Urbana–Champaign, Champaign, IL, USA;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    Optical filters; Sensors; Dark current; Image sensors; Image quality; Extinction ratio;

    机译:滤光片;传感器;暗电流;图像传感器;图像质量;消光比;

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