OGLE-2016-BLG-1003: First Resolved Caustic-crossing Binary-source Event Discovered by Second-generation Microlensing Surveys
arXiv:1705.01531 · doi:10.3847/1538-4357/aa7057
Abstract
We report the analysis of the first resolved caustic-crossing binary-source microlensing event OGLE-2016-BLG-1003. The event is densely covered by the round-the-clock observations of three surveys. The light curve is characterized by two nested caustic-crossing features, which is unusual for typical caustic-crossing perturbations. From the modeling of the light curve, we find that the anomaly is produced by a binary source passing over a caustic formed by a binary lens. The result proves the importance of high-cadence and continuous observations, and the capability of second-generation microlensing experiments to identify such complex perturbations that are previously unknown. However, the result also raises the issues of the limitations of current analysis techniques for understanding lens systems beyond two masses and of determining the appropriate multiband observing strategy of survey experiments.
7 pages, 6 figures, Accepted for the publication in ApJ
References in corpus (21)
- A method for optimal image subtraction
- Possible Gravitational Microlensing of a Star in the Large Magellanic Cloud
- Reddening and Extinction Toward the Galactic Bulge from OGLE-III: The Inner Milky Way's Rv ~ 2.5 Extinction Curve
- Unbound or Distant Planetary Mass Population Detected by Gravitational Microlensing
- The angular size of dwarf stars and subgiants - Surface brightness relations calibrated by interferometry
- OGLE-2003-BLG-262: Finite-Source Effects from a Point-Mass Lens
- Resolution of the MACHO-LMC-5 Puzzle: The Jerk-Parallax Microlens Degeneracy
- MOA-2011-BLG-293Lb: A test of pure survey microlensing planet detections
- Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars. IV. Two bulge populations
- Binary microlensing event OGLE-2009-BLG-020 gives a verifiable mass, distance and orbit predictions
- Spitzer as Microlens Parallax Satellite: Mass Measurement for the OGLE-2014-BLG-0124L Planet and its Host Star
- The First Circumbinary Planet Found by Microlensing: OGLE-2007-BLG-349L(AB)c
- OGLE-2003-BLG-238: Microlensing Mass Estimate of an Isolated Star
- A Venus-Mass Planet Orbiting a Brown Dwarf: Missing Link between Planets and Moons
- Interpretation of a Short-Term Anomaly in the Gravitational Microlensing Event MOA-2012-BLG-486
- OGLE-2013-BLG-0102LA,B: Microlensing binary with components at star/brown-dwarf and brown-dwarf/planet boundaries
- The First Neptune Analog or Super-Earth with Neptune-like Orbit: MOA-2013-BLG-605Lb
- The Many Possible Interpretations of Microlensing Event OGLE-2002-BLG-055
- Complete Parallax and Proper Motion Solutions For Halo Binary-Lens Microlensing Events
- Binary Source Microlensing Event OGLE-2016-BLG-0733: Interpretation of A Long-term Asymmetric Perturbation
- OGLE-2012-BLG-0455/MOA-2012-BLG-206: Microlensing event with ambiguity in planetary interpretations caused by incomplete coverage of planetary signal
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