Showing 221–240 of 486 results
/ Date/ Name
Jan 28, 2020Constraints on the $K^0_{\mathrm{S}}\rightarrowμ^{+}μ^{-}$ branching fractionJan 23, 2020Mass determinations of the three mini-Neptunes transiting TOI-125Jan 13, 2020First demonstration of OH suppression in a high efficiency near-infrared spectrographJan 6, 2020GW190425: Observation of a Compact Binary Coalescence with Total Mass $\sim 3.4 M_{\odot}$Jan 6, 2020A search for IceCube events in the direction of ANITA neutrino candidatesJan 3, 2020A Joint Fermi-GBM and LIGO/Virgo Analysis of Compact Binary Mergers From the First and Second Gravitational-wave Observing RunsDec 25, 2019Open data from the first and second observing runs of Advanced LIGO and Advanced VirgoDec 17, 2019The HI/OH/Recombination line survey of the inner Milky Way (THOR): data release 2 and HI overviewNov 8, 2019Measurement of the $η_c(1S)$ production cross-section in $pp$ collisions at $\sqrt{s} = 13$ TeVNov 6, 2019Neutrino astronomy with the next generation IceCube Neutrino ObservatoryOct 24, 2019Measurement of $\mathitΞ_{cc}^{++}$ production in $pp$ collisions at $\sqrt{s}=13$ TeVOct 15, 2019Design and Performance of the first IceAct Demonstrator at the South PoleOct 14, 2019Revealing the Origin and Cosmic Evolution of Supermassive Black HolesSep 4, 2019Efficient propagation of systematic uncertainties from calibration to analysis with the SnowStorm method in IceCubeAug 29, 2019A guide to LIGO-Virgo detector noise and extraction of transient gravitational-wave signalsAug 27, 2019A Search for MeV to TeV Neutrinos from Fast Radio Bursts with IceCubeAug 26, 2019Search for PeV Gamma-Ray Emission from the Southern Hemisphere with 5 Years of Data from the IceCube ObservatoryJul 29, 2019Velocity independent constraints on spin-dependent DM-nucleon interactions from IceCube and PICOJul 15, 2019Search for Sources of Astrophysical Neutrinos Using Seven Years of IceCube Cascade EventsJul 8, 2019Space Telescope and Optical Reverberation Mapping Project. VIII. Time Variability of Emission and Absorption in NGC 5548 Based on Modeling the Ultraviolet Spectrum