Showing 21–40 of 42 results
/ Date/ Name
Mar 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 DataJul 30, 2020Orbital angular momentum beam generation using a free-electron laser oscillatorJan 27, 2020Prospects for Fundamental Physics with LISANov 19, 2019Particle Physics with the Cosmic Microwave Background with SPT-3GMar 21, 2019Gamma Factory at CERN -- novel research tools made of lightMar 12, 2019Messengers from the Early Universe: Cosmic Neutrinos and Other Light RelicsOct 4, 2018Dark Energy Survey Year 1 Results: tomographic cross-correlations between DES galaxies and CMB lensing from SPT+PlanckOct 4, 2018Dark Energy Survey Year 1 Results: Joint Analysis of Galaxy Clustering, Galaxy Lensing, and CMB Lensing Two-point FunctionsAug 31, 2018Year two instrument status of the SPT-3G cosmic microwave background receiverMay 21, 2016Compensation for Booster Leakage Field in the Duke Storage RingApr 16, 2016Study of Magnetic Hysteresis Effects in a Storage Ring Using Precision Tune MeasurementSep 20, 2013Neutrino Physics from the Cosmic Microwave Background and Large Scale StructureApr 19, 2013First Measurements of Spin-Dependent Double-Differential Cross Sections and the GDH Integrand from \vec{^3He}(\vecγ,n)pp at Incident Photon Energies of 12.8 and 14.7 MeVAug 6, 2012Antenna-coupled TES bolometers for the Keck Array, Spider, and Polar-1Jan 24, 2011Theoretical and simulation studies of characteristics of a Compton light sourceFeb 20, 2009Chiral Dynamics in Photo-Pion Physics: Theory, Experiment, and Future Studies at the HI$γ$S FacilitySep 14, 2001The 1998 outburst of XTE J1550-564: a model based on multiwavelength observations