[HTML][HTML] Probing quantum devices with radio-frequency reflectometry
Many important phenomena in quantum devices are dynamic, meaning that they cannot be
studied using time-averaged measurements alone. Experiments that measure such transient …
studied using time-averaged measurements alone. Experiments that measure such transient …
The simons observatory: Astro2020 decadal project whitepaper
MH Abitbol, S Adachi, P Ade, J Aguirre… - arxiv preprint arxiv …, 2019 - arxiv.org
The Simons Observatory (SO) is a ground-based cosmic microwave background (CMB)
experiment sited on Cerro Toco in the Atacama Desert in Chile that promises to provide …
experiment sited on Cerro Toco in the Atacama Desert in Chile that promises to provide …
PICO: Probe of inflation and cosmic origins
The Probe of Inflation and Cosmic Origins (PICO) is an imaging polarimeter that will scan the
sky for 5 years in 21 frequency bands spread between 21 and 799 GHz. It will produce full …
sky for 5 years in 21 frequency bands spread between 21 and 799 GHz. It will produce full …
The Simons observatory: instrument overview
The Simons Observatory (SO) will make precision temperature and polarization
measurements of the cosmic microwave background (CMB) using a series of telescopes …
measurements of the cosmic microwave background (CMB) using a series of telescopes …
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 …
Performance of a kinetic inductance traveling-wave parametric amplifier at 4 kelvin: Toward an alternative to semiconductor amplifiers
Most microwave readout architectures in quantum computing or sensing rely on a
semiconductor amplifier at 4 K, typically a high-electron mobility transistor (HEMT). Despite …
semiconductor amplifier at 4 K, typically a high-electron mobility transistor (HEMT). Despite …
[HTML][HTML] A microwave SQUID multiplexer optimized for bolometric applications
A microwave superconducting quantum interference device multiplexer has been optimized
for reading out large arrays of superconducting transition-edge sensor (TES) bolometers …
for reading out large arrays of superconducting transition-edge sensor (TES) bolometers …
The design of the Ali CMB Polarization Telescope receiver
M Salatino, J Austermann… - … , and Far-Infrared …, 2020 - spiedigitallibrary.org
Publisher's Note: This paper, originally published on 22 December 2020, was replaced with
a corrected/revised version on 12 March 2021. If you downloaded the original PDF but are …
a corrected/revised version on 12 March 2021. If you downloaded the original PDF but are …
[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 …
Prime-Cam: a first-light instrument for the CCAT-prime telescope
CCAT-prime will be a 6-meter aperture telescope operating from sub-mm to mm
wavelengths, located at 5600 meters elevation on Cerro Chajnantor in the Atacama Desert …
wavelengths, located at 5600 meters elevation on Cerro Chajnantor in the Atacama Desert …