[HTML][HTML] Transition edge sensors: Physics and applications
Transition Edge Sensors (TESs) are amongst the most sensitive cryogenic detectors and
can be easily optimized for the detection of massive particles or photons ranging from X-rays …
can be easily optimized for the detection of massive particles or photons ranging from X-rays …
The Simons Observatory: Design, integration, and testing of the small aperture telescopes
Abstract The Simons Observatory (SO) is a cosmic microwave background survey
experiment that includes small-aperture telescopes (SATs) observing from an altitude of …
experiment that includes small-aperture telescopes (SATs) observing from an altitude of …
The Simons Observatory microwave SQUID multiplexing detector module design
Advances in cosmic microwave background (CMB) science depend on increasing the
number of sensitive detectors observing the sky. New instruments deploy large arrays of …
number of sensitive detectors observing the sky. New instruments deploy large arrays of …
SLAC Microresonator RF (SMuRF) Electronics: A tone-tracking readout system for superconducting microwave resonator arrays
C Yu, Z Ahmed, JC Frisch, SW Henderson… - Review of Scientific …, 2023 - pubs.aip.org
We describe the newest generation of the SLAC Microresonator RF (SMuRF) electronics, a
warm digital control and readout system for microwave-frequency resonator-based …
warm digital control and readout system for microwave-frequency resonator-based …
The Simons observatory large aperture telescope receiver
Abstract The Simons Observatory is a ground-based cosmic microwave background
experiment that consists of three 0.4 m small-aperture telescopes and one 6 m Large …
experiment that consists of three 0.4 m small-aperture telescopes and one 6 m Large …
[HTML][HTML] Improved microwave SQUID multiplexer readout using a kinetic-inductance traveling-wave parametric amplifier
We report on the use of a kinetic-inductance traveling-wave parametric amplifier (KITWPA)
as the first amplifier in the readout chain of a microwave superconducting quantum …
as the first amplifier in the readout chain of a microwave superconducting quantum …
Simons Observatory: Predeployment Performance of a Large Aperture Telescope Optics Tube in the 90 and 150 GHz Spectral Bands
CE Sierra, K Harrington, S Sutariya… - The Astrophysical …, 2025 - iopscience.iop.org
Abstract The Simons Observatory will map the temperature and polarization over half of the
sky at millimeter wavelengths in six spectral bands from the Atacama Desert in Chile. These …
sky at millimeter wavelengths in six spectral bands from the Atacama Desert in Chile. These …
Instrumental systematics biases in CMB lensing reconstruction: A simulation-based assessment
Weak gravitational lensing of the cosmic microwave background (CMB) is an important
cosmological tool that allows us to learn about the structure, composition and evolution of …
cosmological tool that allows us to learn about the structure, composition and evolution of …
The Simons Observatory: the large aperture telescope (LAT)
Abstract The Simons Observatory is a Cosmic Microwave Background experiment to
observe the microwave sky in six frequency bands from 30 to 290 GHz. The Observatory …
observe the microwave sky in six frequency bands from 30 to 290 GHz. The Observatory …
High-Dynamic-Range Detection of Microwave Signal on Chip Surface Based on Diamond Sensors
D Wang, HF Wen, X Li, Y **, W Hao… - IEEE Transactions …, 2023 - ieeexplore.ieee.org
This article proposed a microwave (MW) detection method by utilizing the effect of the dual
MW on nitrogen-vacancy (NV) centers in diamond. We established a theoretical model of …
MW on nitrogen-vacancy (NV) centers in diamond. We established a theoretical model of …