An Image Quality Evaluation and Masking Algorithm Based On Pre-trained Deep Neural Networks

TL;DR

This paper introduces a deep learning autoencoder-based algorithm for automatic astronomical image quality evaluation and noise masking, enhancing efficiency and accuracy in data processing pipelines for sky surveys.

Contribution

The study presents a novel autoencoder approach for automatic image quality assessment and noise masking in astronomical data, reducing human intervention and improving processing robustness.

Findings

Effectively identified variations in point spread functions.

Successfully masked complex background regions.

Enhanced photometry accuracy through noise masking.

Abstract

With the growing amount of astronomical data, there is an increasing need for automated data processing pipelines, which can extract scientific information from observation data without human interventions. A critical aspect of these pipelines is the image quality evaluation and masking algorithm, which evaluates image qualities based on various factors such as cloud coverage, sky brightness, scattering light from the optical system, point spread function size and shape, and read-out noise. Occasionally, the algorithm requires masking of areas severely affected by noise. However, the algorithm often necessitates significant human interventions, reducing data processing efficiency. In this study, we present a deep learning based image quality evaluation algorithm that uses an autoencoder to learn features of high quality astronomical images. The trained autoencoder enables automatic evaluation of image quality and masking of noise affected areas. We have evaluated the performance of our algorithm using two test cases: images with point spread functions of varying full width half magnitude, and images with complex backgrounds. In the first scenario, our algorithm could effectively identify variations of the point spread functions, which can provide valuable reference information for photometry. In the second scenario, our method could successfully mask regions affected by complex regions, which could significantly increase the photometry accuracy. Our algorithm can be employed to automatically evaluate image quality obtained by different sky surveying projects, further increasing the speed and robustness of data processing pipelines.