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Recent advances in bioimaging demand application-tailored point spread functions.
Aperture engineering techniques provide interesting solutions for obtaining desired system point spread functions.
Point spread functions have been simulated for both 1D and 2D arrays.
This has practical application, for example when deconvolving microscope images or analyzing point spread functions.
Recovering temporal point spread functions (PSFs) is important for various applications, especially analyzing light transport.
The point spread functions are obtained by a deconvolution technique in the Fourier domain.
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To model the detector response, measured detector line-spread functions were used.
We demonstrated an image-restoration technique using the point-spread functions of stars, and confirmed that the technique functions well in all loss-less images.
The dependability of the various design parameters naturally arises once a relationship between the value of the point-spread functions at the edge of the field-of-view and the pixel field-of-view is introduced.
The Full Width Half Maximum (FWHM) and the Full Width Tenth Maximum (FWTM) of the reconstructed point-spread functions (PSF) were obtained from these images following the NEMA NU2-2012 protocol using in-house software.
Deconvolved images were computed using the point-spread functions and software supplied by the manufacturer.
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