Showing 121–140 of 302 results
/ Date/ Name
Mar 3, 2020Space Telescope and Optical Reverberation Mapping Project. IX. Velocity-Delay Maps for Broad Emission Lines in NGC 5548Jan 6, 2020GW190425: Observation of a Compact Binary Coalescence with Total Mass $\sim 3.4 M_{\odot}$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 21, 2019Contribution of exclusive diffractive processes to the measured azimuthal asymmetries in SIDISNov 21, 2019Low frequency view of GRB 190114C reveals time varying shock micro-physicsSep 6, 2019Probing Majorana neutrinos with double-$β$ decayAug 29, 2019A guide to LIGO-Virgo detector noise and extraction of transient gravitational-wave signalsAug 15, 2019The inter-cluster time synchronization systems within the Baikal-GVD detectorJul 25, 2019Carpet results on astrophysical gamma rays above 100 TeVJul 8, 2019Space Telescope and Optical Reverberation Mapping Project. VIII. Time Variability of Emission and Absorption in NGC 5548 Based on Modeling the Ultraviolet SpectrumJun 19, 2019Search for intermediate mass black hole binaries in the first and second observing runs of the Advanced LIGO and Virgo networkMay 20, 2019Interpolation of equation-of-state dataMar 28, 2019Measurement of the cross section for hard exclusive $π^0$ leptoproductionMar 11, 2019Tests of General Relativity with the Binary Black Hole Signals from the LIGO-Virgo Catalog GWTC-1Feb 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 19, 2019Characterization of 30 $^{76}$Ge enriched Broad Energy Ge detectors for GERDA Phase IIDec 17, 2018Stellar activity analysis of Barnard's Star: Very slow rotation and evidence for long-term activity cycle