OGLE-2013-BLG-1761Lb: A Massive Planet Around an M/K Dwarf
arXiv:1703.07623 · doi:10.3847/1538-3881/aa73da
Abstract
We report the discovery and the analysis of the planetary microlensing event, OGLE-2013-BLG-1761. There are some degenerate solutions in this event because the planetary anomaly is only sparsely sampled. But the detailed light curve analysis ruled out all stellar binary models and shows that the lens to be a planetary system. There is the so-called close/wide degeneracy in the solutions with the planet/host mass ratio of and with the projected separation in Einstein radius units of (close) and (wide), respectively. The microlens parallax effect is not detected but the finite source effect is detected. Our Bayesian analysis indicates that the lens system is located at away from us and the host star is an M/K-dwarf with the mass of orbited by a super-Jupiter mass planet with the mass of at the projected separation of . The preference of the large lens distance in the Bayesian analysis is due to the relatively large observed source star radius. The distance and other physical parameters can be constrained by the future high resolution imaging by ground large telescopes or HST. If the estimated lens distance is correct, this planet provides another sample for testing the claimed deficit of planets in the Galactic bulge.
22pages, 7figures, 2tables, submitted to AAS Journals
References in corpus (15)
- Wide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report
- One or more bound planets per Milky Way star from microlensing observations
- A new implementation of the infrared flux method using the 2MASS catalogue
- Microlens OGLE-2005-BLG-169 Implies Cool Neptune-Like Planets are Common
- A Low-Mass Planet with a Possible Sub-Stellar-Mass Host in Microlensing Event MOA-2007-BLG-192
- The Exoplanet Mass-Ratio Function from the MOA-II Survey: Discovery of a Break and Likely Peak at a Neptune Mass
- MOA-cam3: a wide-field mosaic CCD camera for a gravitational microlensing survey in New Zealand
- Interstellar Extinction Law toward the Galactic Center II: V, J, H, and Ks Bands
- Identification of the OGLE-2003-BLG-235/MOA-2003-BLG-53 Planetary Host Star
- Is the Galactic bulge devoid of planets?
- The Star Blended with the MOA-2008-BLG-310 Source Is Not the Exoplanet Host Star
- OGLE-2008-BLG-355Lb: A Massive Planet around A Late type Star
- Discovery of a Gas giant Planet in Microlensing Event OGLE-2014-BLG-1760
- OGLE-2015-BLG-0051/KMT-2015-BLG-0048Lb: a Giant Planet Orbiting a Low-mass Bulge Star Discovered by High-cadence Microlensing Surveys
- OGLE-2012-BLG-0724Lb: A Saturn-mass Planet around an M-dwarf
Cited by in corpus (6)
- Keck Observations Confirm a Super-Jupiter Planet Orbiting M-dwarf OGLE-2005-BLG-071L
- A Ubiquitous Unifying Degeneracy in Two-Body Microlensing Systems
- A Planetary Microlensing Event with an Unusually Red Source Star: MOA-2011-BLG-291
- OGLE-2016-BLG-0168 Binary Microlensing Event: Prediction and Confirmation of the Micorlens Parallax Effect from Space-based Observation
- OGLE-2015-BLG-1670Lb: A Cold Neptune beyond the Snow Line in the Provisional WFIRST Microlensing Survey Field
- Kmt-2016-blg-1397b: Kmtnet-only discovery of a microlens giant planet