Showing 161–180 of 321 results
/ Date/ Name
Mar 11, 2019Gravity and Light: Combining Gravitational Wave and Electromagnetic Observations in the 2020sMar 11, 2019Tests of General Relativity with the Binary Black Hole Signals from the LIGO-Virgo Catalog GWTC-1Feb 25, 2019Design and Bolometer Characterization of the SPT-3G First-year Focal PlaneFeb 22, 2019Searches for Gravitational Waves from Known Pulsars at Two Harmonics in 2015-2017 LIGO DataFeb 22, 2019Narrow-band search for gravitational waves from known pulsars using the second LIGO observing runFeb 20, 2019Development of an analysis to probe the neutrino mass ordering with atmospheric neutrinos using three years of IceCube DeepCore dataFeb 5, 2019Search for transient gravitational wave signals associated with magnetar bursts during Advanced LIGO's second observing runJan 16, 2019Measurement of Atmospheric Tau Neutrino Appearance with IceCube DeepCoreDec 13, 2018All-Sky Measurement of the Anisotropy of Cosmic Rays at 10 TeV and Mapping of the Local Interstellar Magnetic FieldNov 30, 2018Binary Black Hole Population Properties Inferred from the First and Second Observing Runs of Advanced LIGO and Advanced VirgoOct 12, 2018Physics of nuclei: Key role of an emergent symmetryAug 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 receiverAug 31, 2018Broadband anti-reflective coatings for cosmic microwave background experimentsAug 23, 2018Measurements using the inelasticity distribution of multi-TeV neutrino interactions in IceCubeJul 30, 2018Constraints on Minute-Scale Transient Astrophysical Neutrino SourcesJul 12, 2018Velocity-resolved reverberation mapping of five bright Seyfert 1 galaxiesJul 9, 2018Observation of Reconstructable Radio Emission Coincident with an X-Class Solar Flare in the Askaryan Radio Array Prototype StationJul 5, 2018Differential limit on the extremely-high-energy cosmic neutrino flux in the presence of astrophysical background from nine years of IceCube data