复杂
发表于 2025-3-21 19:14:16
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alabaster
发表于 2025-3-21 23:33:28
Beating the atmosphere,ects, the spreading of the image is determined by the diffraction of light. In practice, for ground-based observatories, the light must pass through the atmosphere, which has a major impact on image quality because of turbulence.
防御
发表于 2025-3-22 03:28:13
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scrutiny
发表于 2025-3-22 08:14:10
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AFFIX
发表于 2025-3-22 11:21:17
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使厌恶
发表于 2025-3-22 13:19:38
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使厌恶
发表于 2025-3-22 20:38:07
Charge-coupled devices,at the dominant detector in modern astronomy is the charge-coupled device (CCD), it is important to consider these remarkable detectors in more detail. We begin with a brief historical review of CCDs from invention to present day, an amazing story by itself, and then cover the basic principles of ho
灯丝
发表于 2025-3-22 21:23:30
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condescend
发表于 2025-3-23 04:54:36
Characterization and calibration of array instruments,tand how the properties of the detector can be measured and how the behavior of the detector affects photometric and spectroscopic analyses. This chapter describes important steps in these calibrations in terms of CCDs, but the same considerations apply to other array detectors. Signal-to-noise expr
树胶
发表于 2025-3-23 07:56:13
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