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James A. Beall (Fed)

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

Proceedings of the 2nd CREST Nano-Virtual-Labs Joint Workshop on Superconductivity

Author(s)
Kent D. Irwin, James A. Beall, W.Bertrand (Randy) Doriese, William Duncan, S. L. Ferreira, Gene C. Hilton, Rob Horansky, John Mates, Nathan A. Tomlin, Galen O'Neil, Carl D. Reintsema, Dan Schmidt, Joel Ullom, Leila R. Vale
Superconductivity is a powerful tool for the detection of electromagnetic radiation and the energy in particle interactions. One leading superconducting

Demonstration of 220/280 GHz Multichroic Feedhorn-Coupled TES Polarimeter

Author(s)
Samantha L. Walker, Carlos E. Sierra, Jason E. Austermann, James A. Beall, Daniel T. Becker, Bradley J. Dober, Shannon M. Duff, Gene C. Hilton, Johannes Hubmayr, Jeffrey L. Van Lanen, Jeff McMahon, Sara M. Simon, Joel N. Ullom, Michael R. Vissers
We describe the design and measurement of feedhorn-coupled, transition-edge sensor (TES) polarimeters with two passbands centered at 220 GHz and 280 GHz

Tile-and-trim micro-resonator array fabrication optimized for high multiplexing factors

Author(s)
Christopher M. McKenney, Jason E. Austermann, James A. Beall, Bradley J. Dober, Shannon M. Duff, Jiansong Gao, Gene C. Hilton, Johannes Hubmayr, Dale Li, Joel N. Ullom, Jeffrey L. Van Lanen, Michael R. Vissers
We present a superconducting micro-resonator array fabrication method that is scalable and reconfigurable and has been optimized for high multiplexing factors

Low-Temperature Detectors for CMB Imaging Arrays

Author(s)
Johannes Hubmayr, Jason E. Austermann, James A. Beall, Daniel T. Becker, Bradley J. Dober, Shannon M. Duff, Jiansong Gao, Gene C. Hilton, Christopher M. McKenney, Joel N. Ullom, Jeffrey L. Van Lanen, Michael R. Vissers
We review advances in low-temperature detector (LTD) arrays for cosmic microwave background (CMB) polarization experiments, with a particular emphasis on

Millimeter-Wave Polarimeters Using Kinetic Inductance Detectors for TolTEC and Beyond

Author(s)
Jason Austermann, James A. Beall, Sean A. Bryan, Bradley Dober, Jiansong Gao, Gene C. Hilton, Johannes Hubmayr, Phillip Mauskopf, Christopher M. McKenney, S M. Simon, Joel Ullom, Michael Vissers, G W. Wilson
Microwave kinetic inductance detectors (MKIDs) provide a compelling path forward to the large-format polarimeter, imaging, and spectrometer arrays needed for
Created October 9, 2019, Updated October 11, 2023