A new method of CCD dark current correction via extracting the dark information from scientific images
Bin Ma, Zhaohui Shang, Yi Hu, Qiang Liu, Lifan Wang, and Peng Wei

TL;DR
This paper introduces a novel method to derive and apply dark current correction frames directly from scientific CCD images, effectively reducing noise and improving photometric accuracy when traditional dark frames are unavailable.
Contribution
The authors present a simple, effective technique to extract dark current information from scientific images, enabling accurate correction without dedicated dark frames, especially useful at high CCD temperatures.
Findings
Dark current correction reduces noise to sky photon noise levels
Method improves photometric precision significantly
Applicable to other projects with similar constraints
Abstract
We have developed a new method to correct dark current at relatively high temperatures for Charge-Coupled Device (CCD) images when dark frames cannot be obtained on the telescope. For images taken with the Antarctic Survey Telescopes (AST3) in 2012, due to the low cooling efficiency, the median CCD temperature was -46C, resulting in a high dark current level of about 3/pix/sec, even comparable to the sky brightness (10/pix/sec). If not corrected, the nonuniformity of the dark current could even overweight the photon noise of the sky background. However, dark frames could not be obtained during the observing season because the camera was operated in frame-transfer mode without a shutter, and the telescope was unattended in winter. Here we present an alternative, but simple and effective method to derive the dark current frame from the scientific images. Then we can…
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