Showing 1–20 of 25 results
/ Date/ Name
Nov 5, 2024Detection of Thermal Emission at Millimeter Wavelengths from Low-Earth Orbit SatellitesApr 2, 2024Mass calibration of DES Year-3 clusters via SPT-3G CMB cluster lensingDec 19, 2024Pointing Accuracy Improvements for the South Pole Telescope with Machine LearningJan 24, 2024candl: Cosmic Microwave Background Analysis with a Differentiable LikelihoodMar 4, 2024First Constraints on the Epoch of Reionization Using the non-Gaussianity of the Kinematic Sunyaev-Zel{'}dovich Effect from the South Pole Telescope and {\it Herschel}-SPIRE ObservationsNov 8, 2024Cosmology From CMB Lensing and Delensed EE Power Spectra Using 2019-2020 SPT-3G Polarization DataOct 28, 2025Towards constraining cosmological parameters with SPT-3G observations of 25% of the skyMar 20, 2026SPT-3G D1: Maps of the millimeter-wave sky from 2019 and 2020 observations of the SPT-3G Main fieldAug 22, 2023A Measurement of Gravitational Lensing of the Cosmic Microwave Background Using SPT-3G 2018 DataMar 21, 2025The SPT-Deep Cluster Catalog: Sunyaev-Zel'dovich Selected Clusters from Combined SPT-3G and SPTpol Measurements over 100 Square DegreesMay 5, 2025Constraints on Inflationary Gravitational Waves with Two Years of SPT-3G DataMar 26, 2024Testing the $\mathbfΛ$CDM Cosmological Model with Forthcoming Measurements of the Cosmic Microwave Background with SPT-3GJan 24, 2024Flaring Stars in a Non-targeted mm-wave Survey with SPT-3GJul 31, 2025SPT-3G D1: Axion Early Dark Energy with CMB experiments and DESIFeb 11, 2026SPT-3G D1: Compton-$y$ maps using data from the SPT-3G and Planck surveysJan 28, 2026SPT-3G D1: A Measurement of Secondary Cosmic Microwave Background Anisotropy PowerJun 25, 2025SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main fieldSep 10, 2025Detection of Millimeter-Wavelength Flares from Two Accreting White Dwarf Systems in the SPT-3G Galactic Plane SurveyJul 30, 2024Measurement and Modeling of Polarized Atmosphere at the South Pole with SPT-3GFeb 10, 2026Measurement of the Full Shape of the Thermal Sunyaev-Zeldovich Power Spectrum from South Pole Telescope and {\it Herschel}-SPIRE Observations