Showing 121–140 of 266 results
/ Date/ Name
Jan 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 13, 2019Neutron-capture elements in dwarf galaxies II: Challenges for the s- and i-processes at low metallicityOct 14, 2019Reflectivity and PDE of VUV4 Hamamatsu SiPMs in Liquid XenonSep 26, 2019The first view of $δ$ Scuti and $γ$ Doradus stars with the TESS missionAug 28, 2019Neutron-capture elements in dwarf galaxies I: Chemical clocks & the short timescale of the r-processAug 15, 2019Measurement of the 3He Spin-Structure Functions and of Neutron (3He) Spin-Dependent Sum Rules at 0.035<Q^2<0.24 GeV^2Jul 25, 2019Elemental and molecular abundances in comet 67P/Churyumov-GerasimenkoJul 16, 2019A comparison between the two lobes of comet 67P/Churyumov-Gerasimenko based on D/H ratios in H2O measured with the Rosetta/ROSINA DFMSJun 19, 2019Search for intermediate mass black hole binaries in the first and second observing runs of the Advanced LIGO and Virgo networkJun 6, 2019Search for Neutrinoless Double-Beta Decay with the Complete EXO-200 DatasetApr 9, 2019The Detailed Science Case for the Maunakea Spectroscopic Explorer, 2019 editionMar 21, 2019Efficient demultiplexed single-photon source with a quantum dot coupled to a nanophotonic waveguideMar 8, 2019Characterization of the Hamamatsu VUV4 MPPCs for nEXONov 26, 2018Double-beta decay of ${}^{130}$Te to the first $0^+$ excited state of ${}^{130}$Xe with CUORE-0Sep 12, 2018Experimental observation of proton bunch modulation in a plasma, at varying plasma densitiesSep 5, 2018ATHOS: On-the-fly stellar parameter determination of FGK stars based on flux ratios from optical spectraJul 17, 2018Planck 2018 results. I. Overview and the cosmological legacy of PlanckJul 11, 2018Krypton isotopes and noble gas abundances in the coma of comet 67P/Churyumov-GerasimenkoJul 10, 2018The R-Process Alliance: Chemical Abundances for a Trio of R-Process-Enhanced Stars -- One Strong, One Moderate, One Mild