Showing 1–20 of 28 results
/ Date/ Name
Feb 5, 2020Observational constraints on the optical and near-infrared emission from the neutron star-black hole binary merger S190814bvDec 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 SurveySep 1, 2016Testing for X-ray-SZ Differences and Redshift Evolution in the X-ray Morphology of Galaxy ClustersApr 26, 2016Supplement: Localization and broadband follow-up of the gravitational-wave transient GW150914Feb 26, 2016Localization and broadband follow-up of the gravitational-wave transient GW150914Apr 24, 2014The Redshift Evolution of the Mean Temperature, Pressure, and Entropy Profiles in 80 SPT-Selected Galaxy ClustersJan 29, 2014Characterization of the Praesepe Star Cluster by Photometry and Proper Motions with 2MASS, PPMXL, and Pan-STARRSOct 14, 2013Cosmological Constraints from Measurements of Type Ia Supernovae discovered during the first 1.5 years of the Pan-STARRS1 SurveyOct 14, 2013Systematic Uncertainties Associated with the Cosmological Analysis of the First Pan-STARRS1 Type Ia Supernova SampleJul 19, 2013A Search for Fast Optical Transients in the Pan-STARRS1 Medium-Deep Survey: M Dwarf Flares, Asteroids, Limits on Extragalactic Rates, and Implications for LSSTMar 6, 2013PS1-10bzj: A Fast, Hydrogen-Poor Superluminous Supernova in a Metal Poor Host GalaxyJan 31, 2013PS1-10afx at z=1.388: Pan-STARRS1 Discovery of a New Type of Superluminous SupernovaMay 29, 2012SPT-CL J0205-5829: A z = 1.32 Evolved Massive Galaxy Cluster in the South Pole Telescope Sunyaev-Zel'dovich Effect SurveyFeb 12, 2009The MACHO Project HST Follow-Up: The Large Magellanic Cloud Microlensing Source StarsAug 31, 2005Hubble Space Telescope Observations of Nine High-Redshift ESSENCE SupernovaeOct 13, 2004Galactic Bulge Microlensing Events from the MACHO CollaborationOct 13, 2004Microlensing Optical Depth towards the Galactic Bulge Using Clump Giants from the MACHO SurveySep 26, 2001Gravitational Microlensing Events Due to Stellar Mass Black HolesFeb 15, 2001The MACHO Project LMC Variable Star Inventory: X. The R Coronae Borealis Stars