Showing 1–20 of 29 results
/ Date/ Name
Mar 1, 2025The Simons Observatory: Science Goals and Forecasts for the Enhanced Large Aperture TelescopeNov 15, 2024BICEP/Keck XIX: Extremely Thin Composite Polymer Vacuum Windows for BICEP and Other High Throughput Millimeter Wave TelescopesSep 3, 2024Development of the 220/270 GHz Receiver of BICEP ArrayMay 29, 2024Constraining Inflation with the BICEP/Keck CMB Polarization ExperimentsOct 16, 2023Results and Limits of Time Division Multiplexing for the BICEP Array High Frequency ReceiversAug 22, 2023A Measurement of Gravitational Lensing of the Cosmic Microwave Background Using SPT-3G 2018 DataFeb 3, 2022Asteroid Measurements at Millimeter Wavelengths with the South Pole TelescopeJun 21, 2021The Design and Integrated Performance of SPT-3GMar 30, 2021Performance and characterization of the SPT-3G digital frequency-domain multiplexed readout system using an improved noise and crosstalk modelMar 25, 2021Constraints on $Λ$CDM Extensions from the SPT-3G 2018 $EE$ and $TE$ Power SpectraMar 10, 2021Detection of Galactic and Extragalactic Millimeter-Wavelength Transient Sources with SPT-3GMar 8, 2021Global 21-cm Cosmology from the Farside of the MoonJan 5, 2021Measurements of the E-Mode Polarization and Temperature-E-Mode Correlation of the CMB from SPT-3G 2018 DataNov 19, 2019Particle Physics with the Cosmic Microwave Background with SPT-3GJul 27, 2019Performance of Al-Mn Transition-Edge Sensor Bolometers in SPT-3GJul 25, 2019On-sky performance of the SPT-3G frequency-domain multiplexed readoutFeb 25, 2019Design and Bolometer Characterization of the SPT-3G First-year Focal PlaneAug 31, 2018Year two instrument status of the SPT-3G cosmic microwave background receiverAug 31, 2018Characterization and performance of the second-year SPT-3G focal planeAug 31, 2018Design and characterization of the SPT-3G receiver