Showing 301–320 of 393 results
/ Date/ Name
Feb 5, 2019Search for transient gravitational wave signals associated with magnetar bursts during Advanced LIGO's second observing runFeb 2, 2019Study of the process $e^+ e^- \to p \bar p$ via initial state radiation at BESIIIJan 31, 2019Higgs Physics at the HL-LHC and HE-LHCDec 27, 2018Measurement of the absolute branching fractions of $Λ_{c}^{+}\toΛηπ^{+}$ and $Σ(1385)^{+}η$Dec 24, 2018Observation of $e^+e^- \rightarrow D_s^+ \overline{D}{}^{(*)0} K^-$ and study of the $P$-wave $D_s$ mesonsDec 14, 2018The Compact Linear Collider (CLIC) - 2018 Summary ReportDec 13, 2018Measurements of the absolute branching fractions and $CP$ asymmetries for $D^+\rightarrow K_{S,L}^0 K^+(π^0)$Nov 30, 2018Binary Black Hole Population Properties Inferred from the First and Second Observing Runs of Advanced LIGO and Advanced VirgoNov 2, 2018Observation of $D^+_s\rightarrow p\bar{n}$ and confirmation of its large branching fractionOct 21, 2018Precision Higgs Physics at CEPCOct 7, 2018Study of the $D^0\to K^-μ^+ν_μ$ dynamics and test of lepton flavor universality with $D^0\to K^-\ell^+ν_\ell$ decaysSep 19, 2018JINGLE, a JCMT legacy survey of dust and gas for galaxy evolution studies: I. Survey overview and first resultsJun 6, 2018Low-$p_T$ $e^{+}e^{-}$ pair production in Au$+$Au collisions at $\sqrt{s_{NN}}$ = 200 GeV and U$+$U collisions at $\sqrt{s_{NN}}$ = 193 GeV at STARMay 15, 2018Search for invisible decays of $ω$ and $φ$ with $J/ψ$ data at BESIIIMay 10, 2018Avatar-Net: Multi-scale Zero-shot Style Transfer by Feature DecorationJan 5, 2018Is the gamma-ray emission around the Coma galaxy cluster a dark matter origin?Dec 8, 2017Numerical methods for the Wigner equation with unbounded potentialOct 16, 2017Follow up of GW170817 and its electromagnetic counterpart by Australian-led observing programsOct 16, 2017Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger ObservatoryOct 16, 2017A gravitational-wave standard siren measurement of the Hubble constant