Showing 1–20 of 23 results
/ Date/ Name
Oct 30, 2017Development of Thermal Kinetic Inductance Detectors suitable for X-ray spectroscopyNov 29, 2021BICEP Array: 150 GHz detector module developmentSep 25, 2025BICEP/Keck XX: Component-separated maps of polarized CMB and thermal dust emission using Planck and BICEP/Keck Observations through the 2018 Observing SeasonMay 29, 2024Constraining Inflation with the BICEP/Keck CMB Polarization ExperimentsMar 30, 2022The Latest Constraints on Inflationary B-modes from the BICEP/Keck TelescopesOct 1, 2021BICEP / Keck XV: The BICEP3 CMB Polarimeter and the First Three Year Data SetOct 14, 2025Improved Absolute Polarization Calibrator for BICEP CMB PolarimetersSep 3, 2024Development of the 220/270 GHz Receiver of BICEP ArrayOct 14, 2022BICEP / Keck XVII: Line of Sight Distortion Analysis: Estimates of Gravitational Lensing, Anisotropic Cosmic Birefringence, Patchy Reionization, and Systematic ErrorsFeb 4, 2021Analysis of Temperature-to-Polarization Leakage in BICEP3 and Keck CMB Data from 2016 to 2018Jan 25, 2018Al/Ti/Al phonon-mediated KIDs for UV-VIS light detection over large areasJul 29, 2022Improved Polarization Calibration of the BICEP3 CMB Polarimeter at the South PoleOct 1, 2021BICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing SeasonDec 17, 2020Observing low elevation sky and the CMB Cold Spot with BICEP3 at the South PoleAug 4, 2022Thermal Testing for Cryogenic CMB Instrument Optical DesignOct 16, 2023Results and Limits of Time Division Multiplexing for the BICEP Array High Frequency ReceiversOct 15, 2024BICEP/Keck XVIII: Measurement of BICEP3 polarization angles and consequences for constraining cosmic birefringence and inflationOct 11, 2022BICEP / Keck XVI: Characterizing Dust Polarization through Correlations with Neutral HydrogenAug 1, 20222022 Upgrade and Improved Low Frequency Camera Sensitivity for CMB Observation at the South PoleAug 6, 2021BICEP / Keck XIV: Improved constraints on axion-like polarization oscillations in the cosmic microwave background