Showing 1–20 of 42 results
/ Date/ Name
Mar 14, 2021Anti-reflection Coated Vacuum Window for the Primordial Inflation Polarization ExploreR (PIPER) balloon-borne instrumentNov 5, 2018The Atacama Cosmology Telescope: Two-season ACTPol Extragalactic Point Sources and their Polarization propertiesAug 25, 2023Cosmology Large Angular Scale Surveyor (CLASS): 90 GHz Telescope Pointing, Beam Profile, Window Function, and Polarization PerformanceJan 30, 2014Horn Coupled Multichroic Polarimeters for the Atacama Cosmology Telescope Polarization ExperimentDec 2, 2022Characterization of Low-noise Backshort-Under-Grid Kilopixel Transition Edge Sensor Arrays for PIPERAug 9, 2022Cosmology Large Angular Scale Surveyor (CLASS): Pointing Stability and Beam Measurements at 90, 150, and 220 GHzOct 24, 2020Venus Observations at 40 and 90 GHz with CLASSJul 14, 2020The Atacama Cosmology Telescope: DR4 Maps and Cosmological ParametersDec 1, 2014The Atacama Cosmology Telescope: Lensing of CMB Temperature and Polarization Derived from Cosmic Infrared Background Cross-CorrelationNov 29, 2016The Atacama Cosmology Telescope: Two-Season ACTPol Lensing Power SpectrumDec 18, 2020Optical Design of the EXperiment for Cryogenic Large-Aperture Intensity Mapping (EXCLAIM)Jan 21, 2025A Measurement of the Largest-Scale CMB E-mode Polarization with CLASSDec 31, 2020Two Year Cosmology Large Angular Scale Surveyor (CLASS) Observations: Long Timescale Stability Achieved with a Front-End Variable-delay Polarization Modulator at 40 GHzAug 1, 2019The CLASS 150/220 GHz Polarimeter Array: Design, Assembly, and CharacterizationMay 13, 2022Calibration of Transition-edge Sensor (TES) Bolometer Arrays with Application to CLASSAug 9, 2022Construction of a Large Diameter Reflective Half-Wave Plate Modulator for Millimeter Wave ApplicationsNov 28, 2014Evidence of Lensing of the Cosmic Microwave Background by Dark Matter HalosSep 17, 2017The Atacama Cosmology Telescope: The Two-Season ACTPol Sunyaev-Zel'dovich Effect Selected Cluster CatalogNov 19, 2024High-Efficiency and Low-Noise Detectors for the Upgraded CLASS 90 GHz Focal PlaneSep 1, 2023CLASS Angular Power Spectra and Map-Component Analysis for 40 GHz Observations through 2022