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• W3100836417 abstract "Context. One of the possible approaches to detecting optical counterparts of GRBs requires monitoring large parts of the sky. This idea has gained some instrumental support in recent years, such as with the “Pi of the Sky” project. The broad sky coverage of the “Pi of the Sky” apparatus results from using cameras with wide-angle lenses (20° × 20° field of view). Optics of this kind introduce significant deformations of the point spread function (PSF), increasing with the distance from the frame centre. A deformed PSF results in additional uncertainties in data analysis." @default.
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• W3100836417 date "2013-03-01" @default.
• W3100836417 modified "2023-10-18" @default.
• W3100836417 title "PSF modelling for very wide-field CCD astronomy" @default.
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• W3100836417 doi "https://doi.org/10.1051/0004-6361/201219230" @default.
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