摘要: In this article, we provide an alternative up-sampling and PSF deconvolution
method for the iterative multi-exposure coaddition. Different from the previous
works, the new method has a ratio-correction term, which allows the iterations
to converge more rapidly to an accurate representation of the underlying image
than those with difference-correction terms. By employing this method, one can
coadd the under-sampled multi-exposures to a super-resolution and obtain a
higher peak signal-to-noise ratio. A set of simulations show that we can take
many advantages of the new method, e.g. in the signal-to-noise ratio, the
average deviation of all source fluxes, super-resolution, and source distortion
ratio, etc., which are friendly to astronomical photometry and morphology, and
benefits faint source detection and shear measurement of weak gravitational
lensing. It provides an improvement in fidelity over the previous works tested
in this paper.