Showing 21–40 of 66 results
/ Date/ Name
Jul 2, 2015Prime Focus Spectrograph for the Subaru telescope: massively multiplexed optical and near-infrared fiber spectrographMar 15, 2005Astrophysical Observations: Lensing and Eclipsing Einstein's TheoriesJun 13, 2013The Submillimeter Polarization Spectrum of M17Aug 12, 2014Progress with the Prime Focus Spectrograph for the Subaru Telescope: a massively multiplexed optical and near-infrared fiber spectrographJul 21, 2016The Primordial Inflation Polarization Explorer (PIPER)Nov 16, 2015Fabrication of Feedhorn-Coupled Transition Edge Sensor Arrays for Measurement of the Cosmic Microwave Background PolarizationJan 31, 2002Journey to the edge of time: The GREAT missionJul 16, 2021Four-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: On-sky Receiver Performance at 40, 90, 150, and 220 GHz Frequency BandsNov 4, 2019Two-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: A First Detection of Atmospheric Circular Polarization at Q BandNov 19, 2018On-sky performance of the CLASS Q-band telescopeJul 31, 2015Measuring the Largest Angular Scale CMB B-mode Polarization with Galactic Foregrounds on a Cut SkyApr 24, 2020Full-sky Cosmic Microwave Background Foreground Cleaning Using Machine LearningApr 2, 2021Limits on Polarized Dust Spectral Index Variations for CMB Foreground AnalysisAug 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 7, 2022Novel infrared-blocking aerogel scattering filters and their applications in astrophysical and planetary scienceAug 9, 2022Construction of a Large Diameter Reflective Half-Wave Plate Modulator for Millimeter Wave ApplicationsAug 20, 2014Scalable background-limited polarization-sensitive detectors for mm-wave applicationsNov 19, 2024High-Efficiency and Low-Noise Detectors for the Upgraded CLASS 90 GHz Focal PlaneJan 13, 2011A method to extract the redshift distortions beta parameter in configuration space from minimal cosmological assumptions