Showing 1–19 of 19 results
/ Date/ Name
Dec 10, 2024Multiprobe Cosmology from the Abundance of SPT Clusters and DES Galaxy Clustering and Weak LensingNov 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-3GJan 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-3GMar 12, 2019Messengers from the Early Universe: Cosmic Neutrinos and Other Light RelicsOct 4, 2018Dark Energy Survey Year 1 Results: tomographic cross-correlations between DES galaxies and CMB lensing from SPT+PlanckOct 4, 2018Dark Energy Survey Year 1 Results: Joint Analysis of Galaxy Clustering, Galaxy Lensing, and CMB Lensing Two-point FunctionsAug 31, 2018Year two instrument status of the SPT-3G cosmic microwave background receiverSep 20, 2013Neutrino Physics from the Cosmic Microwave Background and Large Scale StructureAug 6, 2012Antenna-coupled TES bolometers for the Keck Array, Spider, and Polar-1