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Title: Fabrication of large dual-polarized multichroic TES bolometer arrays for CMB measurements with the SPT-3G camera

Journal Article · · Superconductor Science and Technology
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  1. Argonne National Lab. (ANL), Argonne, IL (United States)
  2. Cardiff Univ. (United Kingdom)
  3. Stanford Univ., CA (United States); SLAC National Accelerator Lab., Menlo Park, CA (United States)
  4. Univ. of California, San Diego, CA (United States)
  5. Univ. of Colorado, Boulder, CO (United States); National Inst. of Standards and Technology (NIST), Boulder, CO (United States). Quantum Devices Group
  6. Argonne National Lab. (ANL), Argonne, IL (United States); Univ. of Chicago, IL (United States)
  7. Univ. of Chicago, IL (United States); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
  8. SLAC National Accelerator Lab., Menlo Park, CA (United States)
  9. McGill Univ., Montreal, QC (Canada)
  10. Univ. of Chicago, IL (United States)
  11. Univ. of California, Berkeley, CA (United States)
  12. Argonne National Lab. (ANL), Argonne, IL (United States). Center for Nanoscale Materials
  13. McGill Univ., Montreal, QC (Canada); Canadian Inst. for Advanced Research (CIFAR), Toronto, ON (Canada)
  14. Univ. of Colorado, Boulder, CO (United States)
  15. High Energy Accelerator Research Organization (KEK), Tsukuba (Japan)
  16. National Inst. of Standards and Technology (NIST), Boulder, CO (United States). Quantum Devices Group
  17. Stanford Univ., CA (United States)
  18. Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
  19. Univ. of California, Berkeley, CA (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
  20. Univ. of Illinois at Urbana-Champaign, IL (United States)
  21. California Inst. of Technology (CalTech), Pasadena, CA (United States)
  22. Case Western Reserve Univ., Cleveland, OH (United States)
  23. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
  24. Three-Speed Logic, Inc., Vancouver, BC (Canada)
  25. Univ. of Toronto, ON (Canada)

This paper presents the procedures used by Argonne National Laboratory to fabricate large arrays of multichroic transition-edge sensor (TES) bolometers for cosmic microwave background (CMB) measurements. These detectors will be assembled into the focal plane for the SPT-3G camera, the third generation CMB camera to be installed in the South Pole Telescope. The complete SPT-3G camera will have approximately 2690 pixels, for a total of 16,140 TES bolometric detectors. Each pixel is comprised of a broad-band sinuous antenna coupled to a Nb microstrip line. In-line filters are used to define the different band-passes before the millimeter-wavelength signal is fed to the respective Ti/Au TES bolometers. There are six TES bolometer detectors per pixel, which allow for measurements of three band-passes (95 GHz, 150 GHz and 220 GHz) and two polarizations. The steps involved in the monolithic fabrication of these detector arrays are presented here in detail. Patterns are defined using a combination of stepper and contact lithography. The misalignment between layers is kept below 200 nm. The overall fabrication involves a total of 16 processes, including reactive and magnetron sputtering, reactive ion etching, inductively coupled plasma etching and chemical etching.

Research Organization:
Univ. of Illinois at Urbana-Champaign, IL (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP); USDOE Office of Science (SC), Basic Energy Sciences (BES); National Science Foundation (NSF); Kavli Foundation; Gordon and Betty Moore Foundation
Grant/Contract Number:
SC0015640; AC02-06CH11357; ANT-0638937; PHY-1125897; AST-0956135; AST-1402161
OSTI ID:
1594616
Alternate ID(s):
OSTI ID: 1238854
Journal Information:
Superconductor Science and Technology, Vol. 28, Issue 9; ISSN 0953-2048
Publisher:
IOP PublishingCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 30 works
Citation information provided by
Web of Science

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