Showing 181–200 of 652 results
/ Date/ Name
Jul 7, 2021Search for High-Energy Neutrinos from Ultra-Luminous Infrared Galaxies with IceCubeMay 27, 2021Constraints on dark photon dark matter using data from LIGO's and Virgo's third observing runMay 13, 2021Search for lensing signatures in the gravitational-wave observations from the first half of LIGO-Virgo's third observing runMay 5, 2021TESS and HARPS reveal two sub-Neptunes around TOI 1062Apr 30, 2021TOI-269 b: An eccentric sub-Neptune transiting a M2 dwarf revisited with ExTrAApr 28, 2021Probing transversity by measuring $Λ$ polarisation in SIDISApr 26, 2021Projected sensitivity of the LUX-ZEPLIN (LZ) experiment to the two-neutrino and neutrinoless double beta decays of $^{134}$XeApr 15, 2021SALT3: An Improved Type Ia Supernova Model for Measuring Cosmic DistancesMar 31, 2021A muon-track reconstruction exploiting stochastic losses for large-scale Cherenkov detectorsMar 10, 2021Triboelectric Backgrounds to radio-based UHE Neutrino ExeperimentsMar 1, 2021Surface detectors of the TAx4 experimentFeb 23, 2021Projected sensitivities of the LUX-ZEPLIN (LZ) experiment to new physics via low-energy electron recoilsJan 14, 2021SN 2013ai: a link between hydrogen-rich and hydrogen-poor core-collapse supernovaeJan 12, 2021A hot mini-Neptune in the radius valley orbiting solar analogue HD 110113Dec 23, 2020Diving below the spin-down limit: Constraints on gravitational waves from the energetic young pulsar PSR J0537-6910Dec 22, 2020All-sky search in early O3 LIGO data for continuous gravitational-wave signals from unknown neutron stars in binary systemsDec 7, 2020Comparison of $pp$ and $p \bar{p}$ differential elastic cross sections and observation of the exchange of a colorless $C$-odd gluonic compoundOct 31, 2020Searches for 25 rare and forbidden decays of $D^+$ and $D_s^+$ mesonsOct 27, 2020Tests of General Relativity with Binary Black Holes from the second LIGO-Virgo Gravitational-Wave Transient CatalogOct 27, 2020GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run