research
∙
11/20/2020
Compressive Shack-Hartmann Wavefront Sensing based on Deep Neural Networks
The Shack-Hartmann wavefront sensor is widely used to measure aberration...
share
research
∙
11/07/2020
Data–driven Image Restoration with Option–driven Learning for Big and Small Astronomical Image Datasets
Image restoration methods are commonly used to improve the quality of as...
research
∙
03/02/2020
PSF–NET: A Non-parametric Point Spread Function Model for Ground Based Optical Telescopes
Ground based optical telescopes are seriously affected by atmospheric tu...
research
∙
01/31/2020
Point Spread Function Modelling for Wide Field Small Aperture Telescopes with a Denoising Autoencoder
The point spread function reflects the state of an optical telescope and...
research
∙
07/29/2019
Solar Image Restoration with the Cycle-GAN Based on Multi-Fractal Properties of Texture Features
Texture is one of the most obvious characteristics in solar images and i...
research
∙
05/24/2019
Perception Evaluation -- A new solar image quality metric based on the multi-fractal property of texture features
Next-generation ground-based solar observations require good image quali...
research
∙
04/29/2019