Prototype finline-coupled TES bolometers for CLOVER
Michael D. Audley, Robert W. Barker, Michael Crane, Roger Dace, Dorota, Glowacka, David J. Goldie, Anthony N. Lasenby, Howard M. Stevenson, Vassilka, Tsaneva, Stafford Withington, Paul Grimes, Bradley Johnson, Ghassan Yassin,, Lucio Piccirillo, Giampaolo Pisano

TL;DR
This paper presents the design, fabrication, and initial testing of finline-coupled TES bolometers for the CLOVER experiment, aiming to detect B-mode polarization of the cosmic microwave background.
Contribution
It introduces a novel detector design for CLOVER, including fabrication, readout, and preliminary performance validation of prototype detectors.
Findings
Detectors operate successfully at 230 mK with target NEPs.
Prototype detectors validate the design and readout approach.
Initial measurements show promising performance for CMB polarization detection.
Abstract
CLOVER is an experiment which aims to detect the signature of gravitational waves from inflation by measuring the B-mode polarization of the cosmic microwave background. CLOVER consists of three telescopes operating at 97, 150, and 220 GHz. The 97-GHz telescope has 160 feedhorns in its focal plane while the 150 and 220-GHz telescopes have 256 horns each. The horns are arranged in a hexagonal array and feed a polarimeter which uses finline-coupled TES bolometers as detectors. To detect the two polarizations the 97-GHz telescope has 320 detectors while the 150 and 220-GHz telescopes have 512 detectors each. To achieve the target NEPs (1.5, 2.5, and 4.5x10^-17 W/rtHz) the detectors are cooled to 100 mK for the 97 and 150-GHz polarimeters and 230 mK for the 220-GHz polarimeter. Each detector is fabricated as a single chip to ensure a 100% operational focal plane. The detectors are contained…
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Taxonomy
TopicsSuperconducting and THz Device Technology · Physics of Superconductivity and Magnetism · solar cell performance optimization
