We investigated a method for handling GD in the absence of calibration observations. This method requires only several frames with a dozen reference stars to derive an accurate GD solution, so that it can be used for solving GD of some telescopes which were intractable in the past.
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We investigated a method for handling GD in the absence of calibration observations. This method requires only several frames with a dozen reference stars to derive an accurate GD solution, so that it can be used for solving GD of some telescopes which were intractable in the past.
JxnuLin/GDSolver
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We investigated a method for handling GD in the absence of calibration observations. This method requires only several frames with a dozen reference stars to derive an accurate GD solution, so that it can be used for solving GD of some telescopes which were intractable in the past.
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