Attainment of diffraction limited resolution in large telescopes by Fourier analysing speckle patterns in star images

TL;DR: Two simple models of speckle imaging are led that involve neither details of the recovery procedure nor of the atmospheric behavior (except for the size of the seeing disk) and are governed by a dimensionless ratio that involves all parameters relevant to the process of image restoration.

TL;DR: In this paper, the authors used Generalized Cross Validation (GCV) to validate their work and received many helpful feedbacks from the readers of their papers, such as Lalaké Apoyan pointed out the scintillation effects of turbulence, and Dr. Steven Simske from HP lab for his support and encouragement throughout my program.

TL;DR: In this paper, the authors presented two image processing methods, both based on an inverse problem approach, enabling disentanglement of the quasi-static speckles from the planetary signals.

TL;DR: This work proposes a new, modified version of speckle masking that is based on cross triple correlation processing (or cross bispectrum processing) instead of autotriple correlation processing, and shows computer simulations that illustrate the feasibility of the method.