KMT-2021-BLG-0322: Severe degeneracy between triple-lens and higher-order binary-lens interpretations
arXiv:2109.02210 · doi:10.1051/0004-6361/202141939
Abstract
We investigate the microlensing event KMT-2021-BLG-0322, for which the light curve exhibits three distinctive sets of caustic-crossing features. It is found that the overall features of the light curve are approximately described by a binary-lens (2L1S) model, but the model leaves substantial residuals. We test various interpretations with the aim of explaining the residuals. We find that the residuals can be explained either by considering a nonrectilinear lens-source motion caused by the microlens-parallax and lens-orbital effects or by adding a low-mass companion to the binary lens (3L1S model). The degeneracy between the higher-order 2L1S model and the 3L1S model is very severe, making it difficult to single out a correct solution based on the photometric data. This degeneracy was known before for two previous events (MACHO-97-BLG-41 and OGLE-2013-BLG-0723), which led to the false detections of planets in binary systems, and thus the identification of the degeneracy for KMT-2021-BLG-0322 illustrates that the degeneracy can be not only common but also very severe, emphasizing the need to check both interpretations of deviations from 2L1S models. From the Bayesian analysis conducted with the measured lensing observables of the event timescale, angular Einstein radius, and microlens parallax, it was estimated that the binary lens components have masses , for both 2L1S and 3L1S solutions, and the mass of the tertiary lens component according to the 3L1S solution is .
9 pages, 10 figures, 3 tables
References in corpus (34)
- A method for optimal image subtraction
- Long-Term Stability of Planets in Binary Systems
- Reddening and Extinction Toward the Galactic Bulge from OGLE-III: The Inner Milky Way's Rv ~ 2.5 Extinction Curve
- Real-Time Difference Imaging Analysis of MOA Galactic Bulge Observations During 2000
- Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars. V. Evidence for a wide age distribution and a complex MDF
- 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
- The Use of High Magnification Microlensing Events in Discovering Extra-solar Planets
- Expanding the Realm of Microlensing Surveys with Difference Image Photometry
- A Natural Formalism for Microlensing
- Exoplanet Statistics and Theoretical Implications
- MOA-2011-BLG-293Lb: A test of pure survey microlensing planet detections
- Stellar Contribution to the Galactic Bulge Microlensing Optical Depth
- OGLE-2005-BLG-071Lb, the Most Massive M-Dwarf Planetary Companion?
- MOA-2009-BLG-387Lb: A massive planet orbiting an M dwarf
- The Mass Spectrum Of Machos From Parallax Measurements
- Detection of Rotation in a Binary Microlens: PLANET Photometry of MACHO 97-BLG-41
- Planetary Detection Efficiency of the Magnification 3000 Microlensing Event OGLE-2004-BLG-343
- Korea Microlensing Telescope Network Microlensing Events from 2015: Event-Finding Algorithm, Vetting, and Photometry
- The First Circumbinary Planet Found by Microlensing: OGLE-2007-BLG-349L(AB)c
- A Terrestrial Planet in a ~1 AU Orbit Around One Member of a ~15 AU Binary
- Triple Microlens OGLE-2008-BLG-092L: Binary Stellar System with a Circumprimary Uranus-type Planet
- Gravitational Microlensing Evidence for a Planet Orbiting a Binary Star System
- Properties of Microlensing Light Curve Anomalies Induced by Multiple Planets
- A Venus-Mass Planet Orbiting a Brown Dwarf: Missing Link between Planets and Moons
- Reanalysis of the Gravitational Microlensing Event MACHO-97-BLG-41 based on Combined Data
- OGLE-2016-BLG-0613LABb: A Microlensing Planet in a Binary System
- OGLE-2018-BLG-1700L: Microlensing Planet in Binary Stellar System
- A New Non-Planetary Interpretation of the Microlensing Event OGLE-2013-BLG-0723
- Microlensing Detections of Planets in Binary Stellar Systems
- Effect of a wide binary companion to the lens on the astrometric behavior of gravitational microlensing events
- OGLE-2015-BLG-1771Lb: A Microlens Planet Orbiting an Ultracool Dwarf?
- Kepler Rotation Effects on the Binary-Lens Microlensing Events
- An Earth-mass Planet in a Time of Covid-19: KMT-2020-BLG-0414Lb