Internal response difference correction method for charge coupled device (CCD) pixel
A pixel, difference technology, applied in the field of astronomical data processing, can solve the problems of high telescope precision requirements, difficult to achieve with small-diameter telescopes, etc., to achieve good results, easy implementation, direct and convenient operation and implementation.
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[0054] (1) Observation equipment: the aperture of the telescope lens is 7 cm, and the CCD model is: ALTA U9000 front-illuminated type with 3056×3056 pixels, and each pixel corresponds to 12.6 arc seconds. The point spread function (PSF) of the star image has a full width at half maximum (FWHM) of 1.2 pixels (corresponding to 1.5 arcseconds).
[0055] (2) Select an observation night with good weather to construct the observation of the two-dimensional correction map of the internal response difference of the pixel, and the specific data collection and processing requirements and processes are carried out according to the requirements described in the "specific implementation mode" of the present invention. The finally obtained two-dimensional correction image of internal response difference of 16 groups of 4×4 pixels is as follows: Figure 4 Shown:
[0056] (3) Select photometric observations at other times, according to the processing steps described in the present invention,...
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