Recent discoveries from the cosmic microwave background: a review of recent progress
Measurements of the anisotropies in the cosmic microwave background (CMB) radiation
have provided a wealth of information about the cosmological model that describes the …
have provided a wealth of information about the cosmological model that describes the …
[HTML][HTML] Transition edge sensors: Physics and applications
M De Lucia, P Dal Bo, E Di Giorgi, T Lari, C Puglia… - Instruments, 2024 - mdpi.com
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 …
Four-year Cosmology Large Angular Scale Surveyor (CLASS) observations: on-sky receiver performance at 40, 90, 150, and 220 GHz frequency bands
Abstract The Cosmology Large Angular Scale Surveyor (CLASS) observes the polarized
cosmic microwave background (CMB) over the angular scales of 1≲ θ≤ 90 with the aim of …
cosmic microwave background (CMB) over the angular scales of 1≲ θ≤ 90 with the aim of …
Calibration of transition-edge sensor (TES) bolometer arrays with application to CLASS
JW Appel, CL Bennett, MK Brewer… - The Astrophysical …, 2022 - iopscience.iop.org
The current and future cosmic microwave background (CMB) experiments fielding kilopixel
arrays of transition-edge sensor (TES) bolometers require accurate and robust gain …
arrays of transition-edge sensor (TES) bolometers require accurate and robust gain …
Design and characterization of the cosmology large angular scale surveyor (CLASS) 93 GHz focal plane
The Cosmology Large Angular Scale Surveyor (CLASS) aims to detect and characterize the
primordial Bmode signal and make a sample-variance-limited measurement of the optical …
primordial Bmode signal and make a sample-variance-limited measurement of the optical …
On-sky performance of new 90 GHz detectors for the Cosmology Large Angular Scale Surveyor (CLASS)
C Núñez, JW Appel, MK Brewer… - IEEE Transactions …, 2023 - ieeexplore.ieee.org
The Cosmology Large Angular Scale Surveyor (CLASS) is a polarization-sensitive
telescope array located at an altitude of 5,200 m in the Chilean Atacama Desert and …
telescope array located at an altitude of 5,200 m in the Chilean Atacama Desert and …
Design and characterization of new 90 GHz detectors for the Cosmology Large Angular Scale Surveyor (CLASS)
The Cosmology Large Angular Scale Surveyor (CLASS) is a polarization-sensitive
telescope array located at an altitude of 5,200 m in the Chilean Atacama Desert. CLASS is …
telescope array located at an altitude of 5,200 m in the Chilean Atacama Desert. CLASS is …
Recent developments of commercially fabricated horn antenna-coupled transition-edge sensor bolometer detectors for next-generation cosmic microwave …
We report on the successful fabrication of orthomode transducer-coupled transition-edge
sensor (TES) bolometer arrays for cosmic microwave background (CMB) polarimetry …
sensor (TES) bolometer arrays for cosmic microwave background (CMB) polarimetry …
Removal of Galactic foregrounds for the Simons Observatory primordial gravitational wave search
Upcoming observations from the Simons Observatory have been projected to constrain the
tensor-to-scalar ratio, $ r $, at the level of $\sigma (r)= $0.003. Here we describe one of the …
tensor-to-scalar ratio, $ r $, at the level of $\sigma (r)= $0.003. Here we describe one of the …
[PDF][PDF] Development of microstrip-coupled lumped-element kinetic inductance detectors for astronomy
A Hornsby - 2020 - core.ac.uk
Abstract Lumped-element Kinetic Inductance Detectors (LEKIDs) are superconducting
Inductor-Capacitor (LC) resonators that have been utilised in large-format arrays of detectors …
Inductor-Capacitor (LC) resonators that have been utilised in large-format arrays of detectors …