Showing 1–20 of 35 results
/ Date/ Name
Nov 14, 2006How random is your heart beat?Jun 26, 2005Statistical and Dynamical Measures of Simple Irreversible ProcessesSep 22, 2004Type I intermittency in a dynamical system with dichotomous parameter changeNov 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 LearningFeb 28, 2023Simultaneous Millimeter-wave, Gamma-ray, and Optical Monitoring of the Blazar PKS 2326-502 During a Flaring StateMar 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 skyApr 2, 2026The South Pole Telescope AGN Monitoring Campaign: First Release of SPTpol Bright AGN Light CurvesMar 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 DataDec 12, 2022A Measurement of the CMB Temperature Power Spectrum and Constraints on Cosmology from the SPT-3G 2018 TT/TE/EE Data SetSep 2, 2025Spectral characterization and performance of SPT-SLIM on-chip filterbank spectrometersOct 9, 2025Probing Anisotropic Cosmic Birefringence with Foreground-Marginalised SPT B-mode LikelihoodsJan 4, 2024SPT Clusters with DES and HST Weak Lensing. II. Cosmological Constraints from the Abundance of Massive HalosMar 21, 2025The SPT-Deep Cluster Catalog: Sunyaev-Zel'dovich Selected Clusters from Combined SPT-3G and SPTpol Measurements over 100 Square DegreesOct 16, 2025An On-Sky Atmospheric Calibration of SPT-SLIMDec 10, 2024Multiprobe Cosmology from the Abundance of SPT Clusters and DES Galaxy Clustering and Weak Lensing