Showing 1–20 of 65 results
/ Date/ Name
Mar 21, 2025The SPT-Deep Cluster Catalog: Sunyaev-Zel'dovich Selected Clusters from Combined SPT-3G and SPTpol Measurements over 100 Square DegreesFeb 10, 2026Measurement of the Full Shape of the Thermal Sunyaev-Zeldovich Power Spectrum from South Pole Telescope and {\it Herschel}-SPIRE ObservationsNov 16, 2020A Demonstration of Improved Constraints on Primordial Gravitational Waves with DelensingJul 3, 2019Fractional Polarisation of Extragalactic Sources in the 500-square-degree SPTpol SurveyJul 19, 2019A Detection of CMB-Cluster Lensing using Polarization Data from SPTpolFeb 28, 2023Simultaneous Millimeter-wave, Gamma-ray, and Optical Monitoring of the Blazar PKS 2326-502 During a Flaring StateApr 2, 2026The South Pole Telescope AGN Monitoring Campaign: First Release of SPTpol Bright AGN Light CurvesJul 22, 2019Galaxy Clusters Selected via the Sunyaev-Zel'dovich Effect in the SPTpol 100-Square-Degree SurveyOct 16, 2019Constraints on Cosmological Parameters from the 500 deg$^2$ SPTpol Lensing Power SpectrumFeb 14, 2020An Improved Measurement of the Secondary Cosmic Microwave Background Anisotropies from the SPT-SZ + SPTpol SurveysJun 15, 2020Searching for Anisotropic Cosmic Birefringence with Polarization Data from SPTpolOct 13, 2019Measurements of B-mode Polarization of the Cosmic Microwave Background from 500 Square Degrees of SPTpol DataJan 11, 2018QUBIC - The Q&U Bolometric Interferometer for Cosmology - A novel way to look at the polarized Cosmic Microwave BackgroundOct 9, 2019The SPTpol Extended Cluster SurveyNov 6, 2018Thermal architecture for the QUBIC cryogenic receiverDec 3, 2020Optimal CMB Lensing Reconstruction and Parameter Estimation with SPTpol DataJul 22, 2013Latest Progress on the QUBIC InstrumentJul 28, 2017Measurements of the Temperature and E-Mode Polarization of the CMB from 500 Square Degrees of SPTpol DataJan 4, 2024SPT Clusters with DES and HST Weak Lensing. II. Cosmological Constraints from the Abundance of Massive HalosDec 10, 2024Multiprobe Cosmology from the Abundance of SPT Clusters and DES Galaxy Clustering and Weak Lensing