Showing 1–20 of 28 results
/ Date/ Name
Dec 10, 2024Multiprobe Cosmology from the Abundance of SPT Clusters and DES Galaxy Clustering and Weak LensingAug 16, 2022Reducing the background in X-ray imaging detectors via machine learningMar 8, 2021Global 21-cm Cosmology from the Farside of the MoonAug 27, 2020CMB-S4: Forecasting Constraints on Primordial Gravitational WavesJun 8, 2020A Multiwavelength Study of the Massive Cool Core Cluster MACS J1447.4+0827Jul 31, 2019CMB-S4 Decadal Survey APC White PaperJul 10, 2019CMB-S4 Science Case, Reference Design, and Project PlanDec 4, 2018Cluster Cosmology Constraints from the 2500 deg$^2$ SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space TelescopeSep 24, 2018A Detailed Study of the Most Relaxed SPT-Selected Galaxy Clusters: Cool Core and Central Galaxy PropertiesNov 16, 2017Hitomi Observation of Radio Galaxy NGC 1275: The First X-ray Microcalorimeter Spectroscopy of Fe-Kα Line Emission from an Active Galactic NucleusOct 12, 2017Measurements of resonant scattering in the Perseus cluster core with Hitomi SXSNov 11, 2016Cluster Mass Calibration at High Redshift: HST Weak Lensing Analysis of 13 Distant Galaxy Clusters from the South Pole Telescope Sunyaev-Zel'dovich SurveySep 21, 2016The First Circumbinary Planet Found by Microlensing: OGLE-2007-BLG-349L(AB)cJun 10, 2016Weighing the Giants V: Galaxy Cluster Scaling RelationsSep 7, 2015Cosmology and astrophysics from relaxed galaxy clusters - IV: Robustly calibrating hydrostatic masses with weak lensingAug 25, 2015Star-Forming Brightest Cluster Galaxies at 0.25 < z < 1.25: A Transitioning Fuel SupplyApr 24, 2014The Redshift Evolution of the Mean Temperature, Pressure, and Entropy Profiles in 80 SPT-Selected Galaxy ClustersJun 4, 2013Probing the extreme realm of AGN feedback in the massive galaxy cluster, RX J1532.9+3021Dec 14, 2012Ripping Apart at the Seams: The Network of Stripped Gas Surrounding M86Nov 23, 2012The rapid evolution of AGN feedback in brightest cluster galaxies: switching from quasar-mode to radio-mode feedback