Amber R. Lennox
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View article: Calibration Measurements of the BICEP3 and BICEP Array CMB Polarimeters from 2017 to 2024
Calibration Measurements of the BICEP3 and BICEP Array CMB Polarimeters from 2017 to 2024 Open
The BICEP3 and BICEP Array polarimeters are small-aperture refracting telescopes located at the South Pole designed to measure primordial gravitational wave signatures in the Cosmic Microwave Background (CMB) polarization, predicted by inf…
View article: In-flight performance of SPIDER's 280 GHz receivers
In-flight performance of SPIDER's 280 GHz receivers Open
SPIDER is a balloon-borne instrument designed to map the cosmic microwave background at degree-angular scales in the presence of Galactic foregrounds. Spider has mapped a large sky area in the Southern Hemisphere using more than 2000 trans…
View article: Plastic Laminate Antireflective Coatings for Millimeter-Wave Optics in BICEP Array
Plastic Laminate Antireflective Coatings for Millimeter-Wave Optics in BICEP Array Open
View article: Improved polarization calibration of the BICEP3 CMB polarimeter at the South Pole
Improved polarization calibration of the BICEP3 CMB polarimeter at the South Pole Open
The BICEP3 Polarimeter is a small aperture, refracting telescope, dedicated to the observation of the Cosmic Microwave Background (CMB) at 95GHz. It is designed to target degree angular scale polarization patterns, in particular the very-m…
View article: Plastic Laminate Antireflective Coatings for Millimeter-wave Optics in BICEP Array
Plastic Laminate Antireflective Coatings for Millimeter-wave Optics in BICEP Array Open
The BICEP/Keck series of experiments target the Cosmic Microwave Background at degree-scale resolution from the South Pole. Over the next few years, the "Stage-3" BICEP Array (BA) telescope will improve the program's frequency coverage and…