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Lauritsen, Lynge; Dickinson, Hugh; Bromley, Jane; Serjeant, Stephen; Lim, Chen-Fatt; Gao, Zhen-Kai and Wang, Wei-Hao
(2021).
DOI: https://doi.org/10.1093/mnras/stab2195
Abstract
Wide-field sub-millimetre surveys have driven many major advances in galaxy evolution in the past decade, but without extensive follow-up observations the coarse angular resolution of these surveys limits the science exploitation. This has driven the development of various analytical deconvolution methods. In the last half a decade Generative Adversarial Networks have been used to attempt deconvolutions on optical data. Here we present an autoencoder with a novel loss function to overcome this problem in the sub-millimeter wavelength range. This approach is successfully demonstrated on Herschel SPIRE 500μm COSMOS data, with the super-resolving target being the JCMT SCUBA-2 450μm observations of the same field. We reproduce the JCMT SCUBA-2 images with high fidelity using this autoencoder. This is quantified through the point source fluxes and positions, the completeness and the purity.
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About
- Item ORO ID
- 78404
- Item Type
- Journal Item
- ISSN
- 1365-2966
- Project Funding Details
-
Funded Project Name Project ID Funding Body ESCAPE - The European Science Cluster of Astronomy & Particle Physics ESFRI Research Infrastructures (EU Horizon 2020 research and innovation programme) 824064 European Union Astronomy at the Open University 2017-2020 ST/P000584/1 Science and Technology Facilities Council STFC Open 2019 DTP ST/T506321/1 Science and Technology Facilities Council - Keywords
- software: data analysis – submillimetre: galaxies – methods: data analysis
- Academic Unit or School
-
Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Faculty of Science, Technology, Engineering and Mathematics (STEM) > Computing and Communications - Research Group
- Astronomy
- Copyright Holders
- © 2021 The Authors.
- Depositing User
- Jane M. Bromley