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James A. Beall (Assoc)

Jim Beall is an Electronics Engineer in the Quantum Devices Group in the Quantum Electromagnetics Division of the Physical Measurement Laboratory at NIST. He has been working at NBS/NIST for over 40 years. His current research interests involve silicon micromachined waveguide structures and superconducting microdevice fabrication process development. Most recently he has led the design, process development and fabrication of micromachined silicon feedhorn and waveguide coupling structures for over 15 fielded microwave detector arrays including ACTpol, AdvACT, Toltec, SPIDER and Simons Observatory. He served as designer and project manager/interface for the construction of 4 clean room facilities at NIST, including the new NIST Boulder Microfabrication Facility and managed the procurement and installation of many large fabrication tools including furnaces, etchers and lithography tools. For several years he managed the Quantum Fabrication Facility. His earlier work included superconducting digital logic circuits, SQUIDs, YBCO thin film junctions and devices, tunable microwave devices, micromachined ion traps, TES detectors and development of photovoltaic devices, III-V tuned-infrared emitters and submicron tungsten-gate GaAs FETs.

RESEARCH INTERESTS

  • Cosmic Microwave Background detector development
  • Microwave feedhorn array development using silicon micromachining
  • Silicon metamaterial lenslet fabrication
  • Silicon micromachining process development

Awards

  • National Institute of Standards and Technology Portrait Gallery (2022)
  • U.S. Department of Commerce Gold Medals (1989, 1993, 2012 and 2021)
  • National Institute of Standards and Technology Bronze Medals (2004 and 2017)
  • National Institute of Standards and Technology Colleagues’ Choice Award (2012)

Publications

Demonstration of a 1,820 channel microwave superconducting quantum1 interference device multiplexer for transition-edge sensor bolometers

Author(s)
John Groh, Jason Austermann, James Beall, Shannon Duff, Johannes Hubmayr, Richard Lew, Michael Link, Tammy Lucas, John Mates, Robinjeet Singh, Joel Ullom, Leila Vale, Jeffrey Van Lanen, Michael Vissers
The scalability of most transition-edge sensor arrays is limited by the multiplexing technology which combines their18 signals over a reduced number of wires

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
Created October 9, 2019, Updated October 11, 2023
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