Brien, T. L. R., Ade, P. ORCID: https://orcid.org/0000-0002-5127-0401, Barry, P. S., Castillo-Dominguez, E., Ferrusca, D., Gomez, V., Hargrave, P. ORCID: https://orcid.org/0000-0002-3109-6629, Hornsby, A. ORCID: https://orcid.org/0000-0002-9998-1720, Hughes, D., Mauskopf, P., Papageorgiou, A., Pascale, E., Rowe, S., Tapia, M., Tucker, C. ORCID: https://orcid.org/0000-0002-1851-3918, Velazquez, M., Ventura, S. and Doyle, S. ORCID: https://orcid.org/0000-0002-9054-986X 2021. Performance and deployment status of MUSCAT: a 1500-pixel LEKID-based mm-wave camera for the large millimeter telescope. Presented at: 45th International Conference on Infrared, Millimeter, and Terahertz Waves (IRMMW-THz), Buffalo, USA, 8-13 Nov 2020. 45th International Conference on Infrared, Millimeter, and Terahertz Waves (IRMMW-THz). 10.1109/IRMMW-THz46771.2020.9370760 |
Abstract
The Mexico-UK Sub-Millimetre Camera for AsTronomy (MUSCAT) is a 1.1-mm band receiver consisting of 1,500 single-colour lumped-element kinetic inductance detectors and is scheduled for deployment to the Large Millimeter Telescope (LMT) after the ongoing COVID-19 pandemic. MUSCAT is designed to utilise the full field of view of the LMT's upgraded 50-m primary mirror (approximately 4′). Here we will present the as-measured performance of MUSCAT from the final lab-verification testing prior to shipping to the LMT. We will also explain the overall design of MUSCAT including the novel technologies utilised—such as continuous cooling using sorption coolers and a miniature dilutor, and horn-coupled LEKIDs—for which MUSCAT will provide a first on-sky demonstration.
Item Type: | Conference or Workshop Item (Paper) |
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Date Type: | Published Online |
Status: | Published |
Schools: | Physics and Astronomy |
ISBN: | 9781728166216 |
ISSN: | 2162-2027 |
Date of First Compliant Deposit: | 9 April 2021 |
Date of Acceptance: | 11 March 2021 |
Last Modified: | 06 Jan 2023 02:10 |
URI: | https://orca.cardiff.ac.uk/id/eprint/140419 |
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