Brien, T. L. R., Ade, P. ![]() ![]() ![]() ![]() ![]() |
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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