Inpainting via Generative Adversarial Networks for CMB data analysis
arXiv:2004.04177 · doi:10.1088/1475-7516/2021/03/012
Abstract
In this work, we propose a new method to inpaint the CMB signal in regions masked out following a point source extraction process. We adopt a modified Generative Adversarial Network (GAN) and compare different combinations of internal (hyper-)parameters and training strategies. We study the performance using a suitable variable in order to estimate the performance regarding the CMB power spectrum recovery. We consider a test set where one point source is masked out in each sky patch with a 1.83 1.83 squared degree extension, which, in our gridding, corresponds to 64 64 pixels. The GAN is optimized for estimating performance on Planck 2018 total intensity simulations. The training makes the GAN effective in reconstructing a masking corresponding to about 1500 pixels with error down to angular scales corresponding to about 5 arcminutes.
arXiv comment19 pages, 21 figures. Prepared for submission to JCAP. All codes will be published after acceptance
References in corpus (7)
- Deep Learning for Real-time Gravitational Wave Detection and Parameter Estimation: Results with Advanced LIGO Data
- Multi-Detector Multi-Component spectral matching and applications for CMB data analysis
- Painting with baryons: augmenting N-body simulations with gas using deep generative models
- DeepSource: Point Source Detection using Deep Learning
- Using inpainting to construct accurate cut-sky CMB estimators
- Cosmic String Detection with Tree-Based Machine Learning
- Predicting CMB dust foreground using galactic 21 cm data
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