The Cosmology Large Angular Scale Surveyor (CLASS) is an experiment to measure the signature of a gravitationalwave background from inflation in the polarization of the cosmic …
J Leech, BK Tan, G Yassin, P Kittara… - IEEE Transactions on …, 2011 - ieeexplore.ieee.org
In previous work, we have described novel smooth-walled multiple flare-angle horns designed using a genetic algorithm. A key feature of these horns is that they can be …
CMB-S4 is a proposed experiment to map the polarization of the Cosmic Microwave Background (CMB) to nearly the cosmic variance limit for angular scales that are accessible …
JR Eimer, Y Li, MK Brewer, R Shi, A Ali… - The Astrophysical …, 2024 - iopscience.iop.org
Measurement of the largest angular scale (ℓ< 30) features of the cosmic microwave background (CMB) polarization is a powerful way to constrain the optical depth to …
In this paper, we present the design, fabrication, and measurements of a lens THz antenna that can be fabricated using conventional photolithography and deep reactive etching …
Z Tao, WX Jiang, HF Ma, TJ Cui - IEEE Transactions on …, 2017 - ieeexplore.ieee.org
A gradient index (GRIN) metamaterial lens antenna with extremely high gain and high aperture efficiency is presented. The proposed antenna is much more advantageous in …
We present the conceptual design of the modular detector and readout system for the Cosmic Microwave Background Stage 4 (CMB-S4) ground-based survey experiment. CMB …
R Datta, MK Brewer, JD Couto, J Eimer… - The Astrophysical …, 2024 - iopscience.iop.org
Abstract The Cosmology Large Angular Scale Surveyor (CLASS) is a telescope array that observes the cosmic microwave background (CMB) over∼ 75% of the sky from the Atacama …
The Cosmology Large Angular Scale Surveyor (CLASS) instrument will measure the polarization of the cosmic microwave background at 40, 90, and 150 GHz from Cerro Toco in …