A Scalable Gaussian Process Approach to Shear Mapping with MuyGPs
Gregory Sallaberry, Benjamin W. Priest, Robert Armstrong, Michael D., Schneider, Amanda Muyskens, Trevor Steil, Keita Iwabuchi

TL;DR
This paper introduces MuyGPs, a scalable Gaussian Process method for shear mapping in cosmic shear analysis, enabling efficient and accurate inference of matter distribution from billions of measurements.
Contribution
The paper presents a novel linear-scaling Gaussian Process approach, MuyGPs, for shear map construction that avoids cubic computational costs by using nearest-neighbor conditioning.
Findings
Accurately interpolates shear maps from simulations.
Recovers two-point and higher order correlations.
Operates efficiently at the scale of billions of galaxies.
Abstract
Analysis of cosmic shear is an integral part of understanding structure growth across cosmic time, which in-turn provides us with information about the nature of dark energy. Conventional methods generate \emph{shear maps} from which we can infer the matter distribution in the universe. Current methods (e.g., Kaiser-Squires inversion) for generating these maps, however, are tricky to implement and can introduce bias. Recent alternatives construct a spatial process prior for the lensing potential, which allows for inference of the convergence and shear parameters given lensing shear measurements. Realizing these spatial processes, however, scales cubically in the number of observations - an unacceptable expense as near-term surveys expect billions of correlated measurements. Therefore, we present a linearly-scaling shear map construction alternative using a scalable Gaussian Process (GP)…
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Taxonomy
TopicsRobotics and Sensor-Based Localization · Image and Object Detection Techniques · Advanced Vision and Imaging
