Showing 1–20 of 21 results
/ Date/ Name
Aug 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-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 PlaneDec 4, 2018Cluster Cosmology Constraints from the 2500 deg$^2$ SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space TelescopeOct 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 receiverAug 31, 2018Characterization and performance of the second-year SPT-3G focal planeAug 31, 2018Design and characterization of the SPT-3G receiverAug 31, 2018Broadband anti-reflective coatings for cosmic microwave background experimentsJul 28, 2014Analysis of Sunyaev-Zel'dovich Effect Mass-Observable Relations using South Pole Telescope Observations of an X-ray Selected Sample of Low Mass Galaxy Clusters and GroupsApr 24, 2014The Redshift Evolution of the Mean Temperature, Pressure, and Entropy Profiles in 80 SPT-Selected Galaxy ClustersDec 26, 2012Constraints on Cosmology from the Cosmic Microwave Background Power Spectrum of the 2500 ${\rm deg}^2$ SPT-SZ Survey