Cleaning Images with Gaussian Process Regression

Abstract

Many approaches to astronomical data reduction and analysis cannot tolerate missing data: corrupted pixels must first have their values imputed. This paper presents astrofix, a robust and flexible image imputation algorithm based on Gaussian Process Regression (GPR). Through an optimization process, astrofix chooses and applies a different interpolation kernel to each image, using a training set extracted automatically from that image. It naturally handles clusters of bad pixels and image edges and adapts to various instruments and image types. For bright pixels, the mean absolute error of astrofix is several times smaller than that of median replacement and interpolation by a Gaussian kernel. We demonstrate good performance on both imaging and spectroscopic data, including the SBIG 6303 0.4m telescope and the FLOYDS spectrograph of Las Cumbres Observatory and the CHARIS integral-field spectrograph on the Subaru Telescope.

Published by the Astronomical Journal. 16 pages, 12 figures. The algorithm is implemented in the Python package astrofix, which is available at https://github.com/HengyueZ/astrofix

References in corpus (3)

• Array Programming with NumPy
• The Gemini Planet Imager: First Light
• Gemini Planet Imager Observational Calibrations I: Overview of the GPI Data Reduction Pipeline

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