Showing 1–20 of 46 results
/ Date/ Name
Dec 17, 2025The Simons Observatory: forecasted constraints on primordial gravitational waves with the expanded array of Small Aperture TelescopesApr 3, 2023Measurement of Dielectric Loss in Silicon Nitride at Centimeter and Millimeter WavelengthsJan 31, 2022Testing low-loss microstrip materials with MKIDs for microwave applicationsJan 5, 2021Measurements of the E-Mode Polarization and Temperature-E-Mode Correlation of the CMB from SPT-3G 2018 DataFeb 5, 2014Nanowire photonic crystal waveguides for single-atom trapping and strong light-matter interactionsDec 12, 2013Atom-Light Interactions in Photonic CrystalsNov 8, 1995Measurement of conditional phase shifts for quantum logicSep 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 3, 2022Asteroid Measurements at Millimeter Wavelengths with the South Pole TelescopeFeb 10, 2026Measurement of the Full Shape of the Thermal Sunyaev-Zeldovich Power Spectrum from South Pole Telescope and {\it Herschel}-SPIRE ObservationsFeb 6, 2026Characterization of the Polarization Beam Response of SPT-3G Using Point SourcesMay 30, 2025Millimeter-wave observations of Euclid Deep Field South using the South Pole Telescope: A data release of temperature maps and catalogsNov 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 LearningMar 10, 2021Detection of Galactic and Extragalactic Millimeter-Wavelength Transient Sources with SPT-3GFeb 28, 2023Simultaneous Millimeter-wave, Gamma-ray, and Optical Monitoring of the Blazar PKS 2326-502 During a Flaring StateJan 22, 2001Characterization of high finesse mirrors: loss, phase shifts and mode structure in an optical cavityMar 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 Observations