Showing 161–180 of 326 results
/ Date/ Name
Jul 27, 2018Measurement of the relative $B^{-} \!\rightarrow D^{0} / D^{*0} / D^{**0} μ^{-} \overlineν_μ$ branching fractions using $B^{-}$ mesons from $\overline{B}{}_{s2}^{*0}$ decaysJul 5, 2018First observation of the doubly charmed baryon decay $Ξ_{cc}^{++}\rightarrow Ξ_{c}^{+}π^{+}$Jul 5, 2018Observation of $B_s^0 \to \overline{D}^{*0} φ$ and search for $B^0 \to \overline{D}^0 φ$ decaysJul 5, 2018Observation of the decay $B_s^0 \to \overline{D}^0 K^+ K^-$Jun 25, 2018Quantum magnetism in molecular spin ladders probed with muon-spin spectroscopyJun 5, 2018Measurement of the time-integrated $CP$ asymmetry in $D^0 \rightarrow K^0_S K^0_S$ decaysJun 4, 2018Measurement of the CKM angle $γ$ using $B^\pm\to DK^\pm$ with $D\to K_\text{S}^0π^+π^-$, $K_\text{S}^0K^+K^-$ decaysMay 24, 2018Measurement of $D_s^{\pm}$ production asymmetry in $pp$ collisions at $\sqrt{s} =7$ and 8 TeVMay 16, 2018Magnetic fields towards Ophiuchus-B derived from SCUBA-2 polarization measurementsMay 9, 2018Measurement of $CP$ violation in $B^{0}\rightarrow D^{\mp}π^{\pm}$ decaysApr 20, 2018GPI spectra of HR 8799 c, d, and e from 1.5 to 2.4$μ$m with KLIP Forward ModelingMar 29, 2018Measurement of the inelastic $pp$ cross-section at a centre-of-mass energy of 13\,TeVFeb 23, 2018Characteristics and energy dependence of recurrent galactic cosmic-ray flux depressions and of a Forbush decrease with LISA PathfinderFeb 15, 2018The properties of Planck Galactic cold clumps in the L1495 dark cloudJan 5, 2018Automated data processing architecture for the Gemini Planet Imager Exoplanet SurveyDec 13, 2017X-ray/UV/optical variability of NGC 4593 with Swift: Reprocessing of X-rays by an extended reprocessorDec 12, 2017Search for excited $B_c^+$ statesDec 8, 2017Updated determination of $D^0$-$\overline{D}{}^0$ mixing and CP violation parameters with $D^0\to K^+π^-$ decaysDec 6, 2017Design and Construction of the DEAP-3600 Dark Matter DetectorNov 12, 2017Laser-only adaptive optics achieves significant image quality gains compared to seeing-limited observations over the entire sky