Showing 1–20 of 21 results
/ Date/ Name
Mar 6, 2025Innovating Bolometers' Mounting: A Gravity-Based ApproachDec 10, 2024Multiprobe Cosmology from the Abundance of SPT Clusters and DES Galaxy Clustering and Weak LensingAug 22, 2023A Measurement of Gravitational Lensing of the Cosmic Microwave Background Using SPT-3G 2018 DataApr 10, 2023A first test of CUPID prototypal light detectors with NTD-Ge sensors in a pulse-tube cryostatMar 16, 2022Toward CUPID-1TFeb 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 27, 2020A CUPID Li$_{2}$$^{100}$MoO$_4$ scintillating bolometer tested in the CROSS underground facilityNov 23, 2020Novel technique for the study of pile-up events in cryogenic bolometersNov 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 PlaneAug 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 receiver