MUSCAT: The Mexico-UK Sub-Millimetre Camera for AsTronomy
Thomas L. R. Brien, Peter A. R. Ade, Peter S. Barry, Edgar, Castillo-Dom\`inguez, Daniel Ferrusca, Thomas Gascard, Victor G\'omez, Peter, C. Hargrave, Amber L. Hornsby, David Hughes, Enzo Pascale, Josie D. A., Parrianen, Abel Perez, Sam Rowe, Carole Tucker

TL;DR
MUSCAT is a large-format sub-millimetre camera for astronomy, utilizing innovative detector and cooling technologies, designed for high-resolution surveys and technology demonstration on the Large Millimeter Telescope.
Contribution
The paper introduces MUSCAT, a novel sub-millimetre camera with innovative design elements like horn-coupled LEKID arrays and continuous cycle refrigeration, serving as both an astronomical instrument and a technology demonstrator.
Findings
Design of continuous sorption refrigerators for stable cooling.
Implementation of broadband optical coupling with waveguide chokes.
Current status of MUSCAT's commissioning process.
Abstract
The Mexico-UK Sub-millimetre Camera for AsTronomy (MUSCAT) is a large-format, millimetre-wave camera consisting of 1,500 background-limited lumped-element kinetic inductance detectors (LEKIDs) scheduled for deployment on the Large Millimeter Telescope (Volc\'an Sierra Negra, Mexico) in 2018. MUSCAT is designed for observing at 1.1 mm and will utilise the full 40' field of view of the LMTs upgraded 50-m primary mirror. In its primary role, MUSCAT is designed for high-resolution follow-up surveys of both galactic and extra-galactic sub-mm sources identified by Herschel. MUSCAT is also designed to be a technology demonstrator that will provide the first on-sky demonstrations of novel design concepts such as horn-coupled LEKID arrays and closed continuous cycle miniature dilution refrigeration. Here we describe some of the key design elements of the MUSCAT instrument such as the novel use…
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