Showing 1–20 of 25 results
/ Date/ Name
Sep 21, 2016The First Circumbinary Planet Found by Microlensing: OGLE-2007-BLG-349L(AB)cJul 10, 2016The radio spectral energy distribution of infrared-faint radio sourcesJan 23, 2015The High Time and Frequency Resolution Capabilities of the Murchison Widefield ArrayJul 17, 2014Study of Redshifted HI from the Epoch of Reionization with Drift scanMar 25, 2014Observing the Sun with the Murchison Widefield ArrayDec 13, 2013A Sub-Earth-Mass Moon Orbiting a Gas Giant Primary or a High Velocity Planetary System in the Galactic BulgeOct 9, 2013A Super-Jupiter orbiting a late-type star: A refined analysis of microlensing event OGLE-2012-BLG-0406Sep 30, 2013MOA-2010-BLG-328Lb: a sub-Neptune orbiting very late M dwarf ?Aug 27, 2013Interpretation of a Short-Term Anomaly in the Gravitational Microlensing Event MOA-2012-BLG-486Aug 13, 2013On the detection and tracking of space debris using the Murchison Widefield Array. I. Simulations and test observations demonstrate feasibilityAug 2, 2013A study of fundamental limitations to statistical detection of redshifted HI from the epoch of reionizationJan 27, 2013The Murchison Widefield Array: solar science with the low frequency SKA PrecursorDec 20, 2012Science with the Murchison Widefield ArrayNov 16, 2012MOA-2010-BLG-073L: An M-Dwarf with a Substellar Companion at the Planet/Brown Dwarf BoundaryApr 13, 2012Characterizing Low-Mass Binaries From Observation of Long Time-scale Caustic-crossing Gravitational Microlensing EventsMar 26, 2012Low Frequency Imaging of Fields at High Galactic Latitude with the Murchison Widefield Array 32-Element PrototypeSep 15, 2011Microlensing Binaries Discovered through High-Magnification ChannelApr 27, 2011OGLE-2005-BLG-018: Characterization of Full Physical and Orbital Parameters of a Gravitational Binary LensSep 28, 2010A frozen super-Earth orbiting a star at the bottom of the Main SequenceMay 6, 2010OGLE 2008--BLG--290: An accurate measurement of the limb darkening of a Galactic Bulge K Giant spatially resolved by microlensing