Showing 1–17 of 17 results
/ Date/ Name
May 22, 2024Euclid: Early Release Observations -- Programme overview and pipeline for compact- and diffuse-emission photometryJun 27, 2020Optical and near-infrared observations of the SPT2349-56 proto-cluster core at z = 4.3Dec 4, 2018Cluster Cosmology Constraints from the 2500 deg$^2$ SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space TelescopeNov 11, 2016Cluster Mass Calibration at High Redshift: HST Weak Lensing Analysis of 13 Distant Galaxy Clusters from the South Pole Telescope Sunyaev-Zel'dovich SurveyMar 16, 2016The redshift distribution of dusty star forming galaxies from the SPT surveyAug 25, 2015Star-Forming Brightest Cluster Galaxies at 0.25 < z < 1.25: A Transitioning Fuel SupplyJul 28, 2014Analysis of Sunyaev-Zel'dovich Effect Mass-Observable Relations using South Pole Telescope Observations of an X-ray Selected Sample of Low Mass Galaxy Clusters and GroupsApr 24, 2014The Redshift Evolution of the Mean Temperature, Pressure, and Entropy Profiles in 80 SPT-Selected Galaxy ClustersSep 12, 2013SPT 0538-50: Physical conditions in the ISM of a strongly lensed dusty star-forming galaxy at z=2.8Mar 11, 2013ALMA redshifts of millimeter-selected galaxies from the SPT survey: The redshift distribution of dusty star-forming galaxiesMar 11, 2013Dusty starburst galaxies in the early Universe as revealed by gravitational lensingJun 20, 2012Submillimeter Observations of Millimeter Bright Galaxies Discovered by the South Pole TelescopeMay 29, 2012SPT-CL J0205-5829: A z = 1.32 Evolved Massive Galaxy Cluster in the South Pole Telescope Sunyaev-Zel'dovich Effect SurveyMay 17, 2011The Hubble Space Telescope Cluster Supernova Survey: V. Improving the Dark Energy Constraints Above z>1 and Building an Early-Type-Hosted Supernova SampleMay 29, 2009The Spitzer Deep, Wide-Field SurveyFeb 17, 2009Mid-Infrared Galaxy Luminosity Functions from the AGN and Galaxy Evolution SurveyAug 10, 2007Low Resolution Spectral Templates For Galaxies From 0.2 -- 10 microns