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Long Wavelength Sensors and Applications Group

The Long Wavelength Sensors and Applications Group develops cryogenic instrumentation for the measurement of faint signals at microwave to far-infrared wavelengths. Applications include precision measurements of Cosmic Microwave Background and other astrophysical observables; quantum sensing; and microwave metrology.

Our group designs and micro-fabricates custom devices that achieve sensitivity at fundamental limits and are based on the principles of superconductivity. We often work in large collaborations to apply these devices to challenging measurements of high scientific interest, such as those which characterize the detailed physical evolution of the universe at large. For more details on our astronomical applications, see Measuring the Cosmos. Terrestrial applications focus on several aspects of microwave metrology, largely in support of quantum measurements. Relevant technologies include transition edge sensor (TES) bolometers, microwave kinetic inductance detectors (MKIDs), SQUID multiplexers, parametric amplifiers, silicon feedhorns, and metamaterial lenslet arrays.

News and Updates

Projects and Programs

Long Wavelength Sensors and Applications

Ongoing
Our project designs and micro-fabricates custom devices that achieve sensitivity at fundamental limits and are based on the principles of superconductivity. We often work in large collaborations to apply these devices to challenging measurements of high scientific interest, such as those which

Publications

280-GHz aluminum MKID arrays for the Fred Young Submillimeter Telescope

Author(s)
Anna Vaskuri, Jordan Wheeler, Jason Austermann, Michael Vissers, James Beall, James R. Burgoyne, Victoria Butler, Scott Chapman, Steve K. Choi, Abigail Crites, Cody J. Duell, Rodrigo Freundt, Anthony Huber, Zachary Huber, Johannes Hubmayr, Jozsef Imrek, Ben Keller, Lawrence Lin, Alicia Middleton, Michael D. Niemack, Thomas Nikola, Douglas Scott, Adrian Sinclair, Ema Smith, Gordon Stacey, Joel Ullom, Jeffrey Van Lanen, Eve Vavagiakis, Samantha Walker, Bugao Zou
First light observations of the 280 GHz instrument module of the Fred Young Submillimeter Telescope (FYST) in the CCAT Collaboration are expected in 2026. The

Awards

Contacts

Group Leader

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