Gómez-Rivera, Víctor, Ade, Peter ![]() ![]() ![]() ![]() ![]() |
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Abstract
MUSCAT is a second-generation continuum camera for the Large Millimeter Telescope (LMT) 'Alfonso Serrano', to observe at the 1.1 mm atmospheric window. The camera has 1500 background-limited, horn-coupled lumped- element kinetic inductance detectors (LEKIDs) split across six arrays operating at 130-mK. The detector design for MUSCAT is based on a large-volume, double-meander geometry used as the inductive and two-polarization absorbing section of the LEKID resonator. In this paper we present the optical coupling of the meander to a choked waveguide output, the microwave design of the LEKID architecture, the device fabrication process and results demonstrating the detector sensitivity under a range of optical loads. Also presented are the performance of an aluminum absorbing layer used to minimize the optical cross-talk between detectors.
Item Type: | Conference or Workshop Item (Paper) |
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Status: | Published |
Schools: | Physics and Astronomy |
Subjects: | Q Science > QB Astronomy Q Science > QC Physics |
Publisher: | SPIE |
Funders: | RCUK, CONACYT |
Date of First Compliant Deposit: | 15 December 2020 |
Date of Acceptance: | 30 November 2020 |
Last Modified: | 27 Oct 2023 06:17 |
URI: | https://orca.cardiff.ac.uk/id/eprint/136983 |
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