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Title: Advanced ACTPol Low-Frequency Array: Readout and Characterization of Prototype 27 and 39 GHz Transition Edge Sensors

Journal Article · · Journal of Low Temperature Physics
ORCiD logo [1];  [2];  [3];  [3];  [4];  [5];  [3];  [4];  [1];  [6];  [1];  [7];  [3];  [1];  [1];  [8]
  1. Cornell Univ., Ithaca, NY (United States). Dept of Physics
  2. Cornell Univ., Ithaca, NY (United States). Dept. of Applied and Engineering Physics
  3. Princeton Univ., NJ (United States). Joseph Henry Lab. of Physics
  4. National Inst. of Standards and Technology (NIST), Boulder, CO (United States). Quantum Devices Group
  5. SLAC National Accelerator Lab., Menlo Park, CA (United States)
  6. Univ. of Pennsylvania, Philadelphia, PA (United States). Dept. of Physics and Astronomy
  7. Univ. of Michigan, Ann Arbor, MI (United States). Dept. of Physics
  8. NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)

Advanced ACTPol (AdvACT) is a third-generation polarization upgrade to the Atacama Cosmology Telescope, designed to observe the cosmic microwave background (CMB). AdvACT expands on the 90 and 150 GHz transition edge sensor (TES) bolometer arrays of the ACT Polarimeter (ACTPol), adding both high-frequency (HF, 150/230 GHz) and low-frequency (LF, 27/39 GHz) multichroic arrays. The addition of the high- and low-frequency detectors allows for the characterization of synchrotron and spinning dust emission at the low frequencies and foreground emission from galactic dust and dusty star-forming galaxies at the high frequencies. The increased spectral coverage of AdvACT will enable a wide range of CMB science, such as improving constraints on dark energy, the sum of the neutrino masses, and the existence of primordial gravitational waves. The LF array will be the final AdvACT array, replacing one of the MF arrays for a single season. Prior to the fabrication of the final LF detector array, we designed and characterized prototype TES bolometers. Detector geometries in these prototypes are varied in order to inform and optimize the bolometer designs for the LF array, which requires significantly lower noise levels and saturation powers (as low as ~1 pW) than the higher-frequency detectors. Here we present results from tests of the first LF prototype TES detectors for AdvACT, including measurements of the saturation power, critical temperature, thermal conductance, and time constants. Finally, we also describe the modifications to the time-division SQUID readout architecture compared to the MF and HF arrays.

Research Organization:
SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
Sponsoring Organization:
USDOE
Grant/Contract Number:
AC02-76SF00515; 1440226; NNX13AE56G; NNX14AB58G; NNX13AL53H
OSTI ID:
1490482
Journal Information:
Journal of Low Temperature Physics, Vol. 193, Issue 5-6; ISSN 0022-2291
Publisher:
Plenum PressCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 13 works
Citation information provided by
Web of Science

References (12)

A SQUID multiplexer with superconducting-to-normalconducting switches journal August 2008
Optical design of the Atacama Cosmology Telescope and the Millimeter Bolometric Array Camera journal January 2007
THE ATACAMA COSMOLOGY TELESCOPE: THE POLARIZATION-SENSITIVE ACTPol INSTRUMENT journal December 2016
Advanced ACTPol Cryogenic Detector Arrays and Readout journal March 2016
Thermal-response time of superconducting transition-edge microcalorimeters journal April 1998
SPIDER: a balloon-borne CMB polarimeter for large angular scales conference July 2010
AlMn Transition Edge Sensors for Advanced ACTPol journal February 2016
Readout of two-kilopixel transition-edge sensor arrays for Advanced ACTPol conference July 2016
Functional Description of Read-out Electronics for Time-Domain Multiplexed Bolometers for Millimeter and Sub-millimeter Astronomy journal January 2008
SPIDER: a balloon-borne CMB polarimeter for large angular scales text January 2011
Advanced ACTPol Cryogenic Detector Arrays and Readout text January 2015
Optical Design of the Atacama Cosmology Telescope and the Millimeter Bolometric Array Camera text January 2007

Cited By (6)

Magnetic Sensitivity of AlMn TESes and Shielding Considerations for Next-Generation CMB Surveys journal May 2018
Developing AlMn Films for Argonne TES Fabrication journal December 2019
The Design of the CCAT-prime Epoch of Reionization Spectrometer Instrument journal January 2020
Demonstration of 220/280 GHz Multichroic Feedhorn-Coupled TES Polarimeter journal January 2020
Developing AlMn films for Argonne TES fabrication text January 2019
The Design of The CCAT-prime Epoch of Reionization Spectrometer Instrument text January 2019

Figures / Tables (5)


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