Challenges
Datasets
Workspaces
Papers
Discussions
Leaderboard
Log inSign up
Challenges
Datasets
Workspaces
Papers
Discussions
Leaderboard
Blog
Job Board
Q3AS

© 2026 Aqora Quantum S.A.S.

TermsPrivacyLegal Notice

Journal of Low Temperature Physics

Recent Developments of Commercially Fabricated Horn Antenna-Coupled Transition-Edge Sensor Bolometer Detectors for Next-Generation Cosmic Microwave Background Polarimetry Experiments

Aritoki Suzuki, Elijah Kane, Adrian Tae-Jin Lee, Tiffany Liu, Christopher Raum, Mario Renzullo, Patrick Truitt, John A. Vivalda, Benjamin Westbrook, Daniel T. Yohannes

Published May 6, 2022• 1 citation
Publisher
DOI
10.1007/s10909-022-02731-x

Related papers

Design and fabrication of superconducting transition edge sensor bolometers with background limited noise performance

Qingya, Zhang, Jian-She +13 more

中国科学通报:英文版•Jan 1, 2014•0 citations

Fabrication of Antenna-Coupled KID Array for Cosmic Microwave Background Detection

Q. Y. Tang, Peter S. Barry, R. Basu Thakur +4 more

arXiv:1710.11255•Journal of Low Temperature Physics•May 10, 2018•5 citations

Developments of Superconducting Microwave Kinetic Inductance Detectors (MKID) for Measurements of Cosmic Microwave Background (CMB) Polarization

S. Mima, Otani Chiko, Kensuke Koga +2 more

IEICE Technical Report; IEICE Tech. Rep.•Apr 12, 2013•0 citations

Optimization of cold resonant filters for frequency domain multiplexed readout of POLARBEAR-2

K. Hattori, Y. Akiba, Kam Arnold +20 more

For the next generation of Cosmic Microwave Background (CMB) experiments, kilopixel arrays of Transition Edge Sensor (TES) bolometers are necessary to achieve the required sensitivity and their science goals. We are developing read-out electronics for POLARBEAR-2 CMB experiment, which multiplexes 32-TES bolometers through a single superconducting quantum interface device (SQUID). To increase both the bandwidth of the SQUID electronics and the multiplexing factor, we are modifying cold wiring and developing LC filters, and a low-inductance superconducting cable. Using these components, we will show frequency domain multiplexing up to 3 MHz.

Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE•Aug 19, 2014•9 citations

Superconducting antenna-coupled YBCO bolometers at submillimeter wavelengths

A. Scheuring, Petra Probst, C. Dischke +2 more

•Jan 1, 2010•0 citations

Microwave SQUID Multiplexer for Cosmic Microwave Background Imagers

Bradley Dober, Daniel Becker, D. A. Bennett +9 more

Key performance characteristics are demonstrated for the microwave SQUID multiplexer ($\mu$MUX) coupled to transition edge sensor (TES) bolometers that have been optimized for cosmic microwave background (CMB) observations. In a 64-channel demonstration, we show that the $\mu$MUX produces a white, input referred current noise level of 29~pA$/\sqrt{\mathrm{Hz}}$ at -77~dB microwave probe tone power, which is well below expected fundamental detector and photon noise sources for a ground-based CMB-optimized bolometer. Operated with negligible photon loading, we measure 98~pA$/\sqrt{\mathrm{Hz}}$ in the TES-coupled channels biased at 65% of the sensor normal resistance. This noise level is consistent with that predicted from bolometer thermal fluctuation (i.e., phonon) noise. Furthermore, the power spectral density exhibits a white spectrum at low frequencies ($\sim$~100~mHz), which enables CMB mapping on large angular scales that constrain the physics of inflation. Additionally, we report cross-talk measurements that indicate a level below 0.3%, which is less than the level of cross-talk from multiplexed readout systems in deployed CMB imagers. These measurements demonstrate the $\mu$MUX as a viable readout technique for future CMB imaging instruments.

•Oct 11, 2017•0 citations
For the next generation of Cosmic Microwave Background (CMB) experiments, kilopixel arrays of Transition Edge Sensor (TES) bolometers are necessary to achieve the required sensitivity and their science goals. We are developing read-out electronics for POLARBEAR-2 CMB experiment, which multiplexes 32-TES bolometers through a single superconducting quantum interface device (SQUID). To increase both the bandwidth of the SQUID electronics and the multiplexing factor, we are modifying cold wiring and developing LC filters, and a low-inductance superconducting cable. Using these components, we will show frequency domain multiplexing up to 3 MHz.
Key performance characteristics are demonstrated for the microwave SQUID multiplexer (μ\muμMUX) coupled to transition edge sensor (TES) bolometers that have been optimized for cosmic microwave background (CMB) observations. In a 64-channel demonstration, we show that the μ\muμMUX produces a white, input referred current noise level of 29~pA/Hz/\sqrt{\mathrm{Hz}}/Hz​ at -77~dB microwave probe tone power, which is well below expected fundamental detector and photon noise sources for a ground-based CMB-optimized bolometer. Operated with negligible photon loading, we measure 98~pA/Hz/\sqrt{\mathrm{Hz}}/Hz​ in the TES-coupled channels biased at 65% of the sensor normal resistance. This noise level is consistent with that predicted from bolometer thermal fluctuation (i.e., phonon) noise. Furthermore, the power spectral density exhibits a white spectrum at low frequencies (∼\sim∼~100~mHz), which enables CMB mapping on large angular scales that constrain the physics of inflation. Additionally, we report cross-talk measurements that indicate a level below 0.3%, which is less than the level of cross-talk from multiplexed readout systems in deployed CMB imagers. These measurements demonstrate the μ\muμMUX as a viable readout technique for future CMB imaging instruments.