Showing 1–20 of 34 results
/ Date/ Name
Oct 22, 2025Quantum computation of molecular geometry via many-body nuclear spin echoesAug 6, 2025Improved limits on the 21cm signal at z=6.5-7.0 with the MWA using Gaussian informationMay 14, 2025Limits on the 21 cm power spectrum at z=6.5-7.0 from MWA observationsFeb 7, 2020Deep multi-redshift limits on Epoch of Reionisation 21cm Power Spectra from Four Seasons of Murchison Widefield Array ObservationsOct 2, 2013Pierre Auger Observatory and Telescope Array: Joint Contributions to the 33rd International Cosmic Ray Conference (ICRC 2013)Nov 28, 2011The Lateral Trigger Probability function for the Ultra-High Energy Cosmic Ray Showers detected by the Pierre Auger ObservatorySep 15, 2011Microlensing Binaries Discovered through High-Magnification ChannelJul 24, 2011The Pierre Auger Observatory I: The Cosmic Ray Energy Spectrum and Related MeasurementsJul 24, 2011The Pierre Auger Observatory III: Other Astrophysical ObservationsApr 27, 2011OGLE-2005-BLG-018: Characterization of Full Physical and Orbital Parameters of a Gravitational Binary LensJan 24, 2011Advanced functionality for radio analysis in the Offline software framework of the Pierre Auger ObservatoryMay 6, 2010OGLE 2008--BLG--290: An accurate measurement of the limb darkening of a Galactic Bulge K Giant spatially resolved by microlensingJul 20, 2009Mass measurement of a single unseen star and planetary detection efficiency for OGLE 2007-BLG-050Feb 12, 2009The MACHO Project HST Follow-Up: The Large Magellanic Cloud Microlensing Source StarsMay 15, 2008LSST: from Science Drivers to Reference Design and Anticipated Data ProductsOct 13, 2004Galactic Bulge Microlensing Events from the MACHO CollaborationOct 13, 2004Microlensing Optical Depth towards the Galactic Bulge Using Clump Giants from the MACHO SurveyOct 15, 2003Probing the atmosphere of a solar-like star by galactic microlensing at high magnificationOct 9, 2003The MACHO Project Large Magellanic Cloud Variable Star Inventory. XIII. Fourier Parameters for the First Overtone RR Lyrae Variables and the LMC DistanceAug 1, 2003The MACHO Project Large Magellanic Cloud variable star inventory. XI. Frequency analysis of the fundamental mode RR Lyrae stars