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Accurate determination of the plate model based on CCD images with different orientations
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作者 PENG QingYu fan liangyan 《Chinese Science Bulletin》 SCIE EI CAS 2010年第9期791-796,共6页
The images of the open cluster NGC2168 are taken using the newly-fitted 2k×2k CCD attached to the 1-m telescope at the Yun-nan Observatory with two different orientations.After the catalogue position of a star fr... The images of the open cluster NGC2168 are taken using the newly-fitted 2k×2k CCD attached to the 1-m telescope at the Yun-nan Observatory with two different orientations.After the catalogue position of a star from UCAC2 is compared with its corresponding measured position,a surprising result shows that a small field of view(about 7′×7′)exhibits an obvious distortion.Spe-cifically,the polynomial between the standard coordinate(ξ,η)and its corresponding measured one(x,y)for a star in each field of view has significant terms as high as 4th order.Accordingly,the positional measurement accuracy of a bright UCAC2 star can be derived as well as~7 mas in each direction(60 s of exposure time and near the zenith).This new finding would be important for a CCD image to deliver a highly accurate position in its whole field of view. 展开更多
关键词 CCD imaging field distortion positional measurement image analysis
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