Showing 1–20 of 24 results
/ Date/ Name
Sep 15, 2011Microlensing Binaries Discovered through High-Magnification ChannelApr 27, 2011OGLE-2005-BLG-018: Characterization of Full Physical and Orbital Parameters of a Gravitational Binary LensMay 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 StarsOct 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 starsJan 29, 2002The MACHO Project LMC Variable Star Inventory: XII. Three Cepheid Variables in Eclipsing BinariesSep 26, 2001Gravitational Microlensing Events Due to Stellar Mass Black HolesFeb 15, 2001The MACHO Project LMC Variable Star Inventory: X. The R Coronae Borealis StarsDec 7, 2000MACHO 96-LMC-2: Lensing of a Binary Source in the LMC and Constraints on the Lensing ObjectNov 28, 2000MACHO Project Limits on Black Hole Dark Matter in the 1-30 Solar Mass RangeSep 26, 2000A 421 d Activity Cycle in the BeX Recurrent Transient A0538-66 from MACHO monitoringMay 23, 2000Galactic Bulge Microlensing Events with Clump Giants as SourcesMay 17, 2000The MACHO Project LMC Variable Star Inventory. IX. Frequency Analysis of the First Overtone RR Lyrae Stars and the Indication for Nonradial PulsationsMar 16, 2000Searching for periodicities in the MACHO light curve of LMC X-2Feb 28, 2000The MACHO project: Microlensing Optical Depth towards the Galactic Bulge from Difference Image Analysis