SRoll3: A neural network approach to reduce large-scale systematic effects in the Planck High Frequency Instrument maps
December 17, 2020 ยท Declared Dead ยท ๐ Astronomy & Astrophysics
"No code URL or promise found in abstract"
Evidence collected by the PWNC Scanner
Authors
Manuel Lรณpez-Radcenco, Jean-Marc Delouis, Laurent Vibert
arXiv ID
2012.09702
Category
astro-ph.IM
Cross-listed
cs.LG
Citations
2
Venue
Astronomy & Astrophysics
Last Checked
1 month ago
Abstract
In the present work, we propose a neural network based data inversion approach to reduce structured contamination sources, with a particular focus on the mapmaking for Planck High Frequency Instrument (Planck-HFI) data and the removal of large-scale systematic effects within the produced sky maps. The removal of contamination sources is rendered possible by the structured nature of these sources, which is characterized by local spatiotemporal interactions producing couplings between different spatiotemporal scales. We focus on exploring neural networks as a means of exploiting these couplings to learn optimal low-dimensional representations, optimized with respect to the contamination source removal and mapmaking objectives, to achieve robust and effective data inversion. We develop multiple variants of the proposed approach, and consider the inclusion of physics informed constraints and transfer learning techniques. Additionally, we focus on exploiting data augmentation techniques to integrate expert knowledge into an otherwise unsupervised network training approach. We validate the proposed method on Planck-HFI 545 GHz Far Side Lobe simulation data, considering ideal and non-ideal cases involving partial, gap-filled and inconsistent datasets, and demonstrate the potential of the neural network based dimensionality reduction to accurately model and remove large-scale systematic effects. We also present an application to real Planck-HFI 857 GHz data, which illustrates the relevance of the proposed method to accurately model and capture structured contamination sources, with reported gains of up to one order of magnitude in terms of contamination removal performance. Importantly, the methods developed in this work are to be integrated in a new version of the SRoll algorithm (SRoll3), and we describe here SRoll3 857 GHz detector maps that will be released to the community.
Community Contributions
Found the code? Know the venue? Think something is wrong? Let us know!
๐ Similar Papers
In the same crypt โ astro-ph.IM
R.I.P.
๐ป
Ghosted
R.I.P.
๐ป
Ghosted
Deep Neural Networks to Enable Real-time Multimessenger Astrophysics
๐
๐
Old Age
Star-galaxy Classification Using Deep Convolutional Neural Networks
R.I.P.
๐ป
Ghosted
CosmoGAN: creating high-fidelity weak lensing convergence maps using Generative Adversarial Networks
R.I.P.
๐ป
Ghosted
Non-negative Matrix Factorization: Robust Extraction of Extended Structures
R.I.P.
๐
404 Not Found
Deep Recurrent Neural Networks for Supernovae Classification
Died the same way โ ๐ป Ghosted
R.I.P.
๐ป
Ghosted
Language Models are Few-Shot Learners
R.I.P.
๐ป
Ghosted
PyTorch: An Imperative Style, High-Performance Deep Learning Library
R.I.P.
๐ป
Ghosted
XGBoost: A Scalable Tree Boosting System
R.I.P.
๐ป
Ghosted