Showing 281–300 of 632 results
/ Date/ Name
May 1, 2019Constraints on Spin-Independent Nucleus Scattering with sub-GeV Weakly Interacting Massive Particle Dark Matter from the CDEX-1B Experiment at the China Jin-Ping LaboratoryApr 11, 2019Final results on neutrino oscillation parameters from the OPERA experiment in the CNGS beamMar 21, 2019Gamma Factory at CERN -- novel research tools made of lightMar 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-1Mar 7, 2019The neutron electric dipole moment experiment at the Spallation Neutron SourceFeb 28, 2019A boron-coated CCD camera for direct detection of Ultracold Neutrons (UCN)Feb 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 5, 2019Search for transient gravitational wave signals associated with magnetar bursts during Advanced LIGO's second observing runJan 31, 2019A next-generation LHC heavy-ion experimentJan 13, 2019MAGIC and Fermi-LAT gamma-ray results on unassociated HAWC sourcesDec 30, 2018The NANOGrav 11-Year Data Set: Limits on Gravitational Waves from Individual Supermassive Black Hole BinariesNov 30, 2018Binary Black Hole Population Properties Inferred from the First and Second Observing Runs of Advanced LIGO and Advanced VirgoNov 30, 2018PEN experiment: a precise test of lepton universalityNov 8, 2018Galaxy inclination and the IRX-beta relation: Effects on UV star-formation rate measurements at intermediate to high redshiftsNov 5, 2018A Jovian planet in an eccentric 11.5 day orbit around HD1397 discovered by TESSNov 3, 2018Hunting for radio emission from the intermittent pulsar J1107-5907 at low frequenciesOct 31, 2018Latest results of the OPERA experiment on nu-tau appearance in the CNGS neutrino beamOct 25, 2018Measurement of the cosmic ray muon flux seasonal variation with the OPERA detector