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OGLE-2017-BLG-0373Lb: A Jovian Mass-Ratio Planet Exposes A New Accidental Microlensing Degeneracy

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Warianty tytułu
Języki publikacji
EN
Abstrakty
EN
We report the discovery of microlensing planet OGLE-2017-BLG-0373Lb. We show that while the planet-host system has an unambiguous microlens topology, there are two geometries within this topology that fit the data equally well, which leads to a factor 2.5 difference in planet-host mass ratio, i.e., q=1.5×10-3 vs. q=0.6×10-3. We show that this is an "accidental degeneracy" in the sense that it is due to a gap in the data. We dub it "the caustic-chirality degeneracy". We trace the mathematical origins of this degeneracy, which should enable similar degenerate solutions to be easily located in the future. A Bayesian estimate, based on a Galactic model, yields a host mass M=0.25+0.30-0.15 M⊙ at a distance DL=5.9+1.3-1.95 kpc. The lens-source relative proper motion is relatively fast, μ=9 mas/yr, which implies that the host mass and distance can be determined by high-resolution imaging after about 10 years. The same observations could in principle resolve the discrete degeneracy in q, but this will be more challenging.
Czasopismo
Rocznik
Strony
43--61
Opis fizyczny
Bibliogr. 41 poz., tab., wykr.
Twórcy
autor
  • Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland
autor
  • Korea Astronomy and Space Science Institute, Daejon 34055, Korea
autor
  • Korea Astronomy and Space Science Institute, Daejon 34055, Korea
autor
  • Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland
  • (OGLE Collaboration)
autor
  • Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland
  • (OGLE Collaboration)
  • Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland
  • (OGLE Collaboration)
  • Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland
  • (OGLE Collaboration)
  • Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland
  • (OGLE Collaboration)
  • Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland
  • (OGLE Collaboration)
autor
  • Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland
  • Department of Astronomy, Ohio State University, 140 W. 18th Ave., Columbus, OH 43210, USA
  • (OGLE Collaboration)
autor
  • Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland
  • (OGLE Collaboration)
autor
  • Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland
  • (OGLE Collaboration)
autor
  • Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland
  • (OGLE Collaboration)
autor
  • Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland
  • (OGLE Collaboration)
autor
  • University of Canterbury, Department of Physics and Astronomy, Private Bag 4800, Christchurch 8020, New Zealand
  • (KMTNet Collaboration)
autor
  • Korea Astronomy and Space Science Institute, Daejon 34055, Korea
  • Korea University of Science and Technology, Daejeon 34113, Korea
  • (KMTNet Collaboration)
autor
  • Korea Astronomy and Space Science Institute, Daejon 34055, Korea
  • Department of Astronomy, Ohio State University, 140 W. 18th Ave., Columbus, OH 43210, USA
  • Max-Planck-Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany
  • (KMTNet Collaboration)
autor
  • Department of Physics, Chungbuk National University, Cheongju 28644, Republic of Korea
  • (KMTNet Collaboration)
autor
  • Harvard-Smithsonian CfA, 60 Garden St., Cambridge, MA 02138, USA
  • (KMTNet Collaboration)
autor
  • Harvard-Smithsonian CfA, 60 Garden St., Cambridge, MA 02138, USA
  • (KMTNet Collaboration)
  • Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA NASA Postdoctoral Program Fellow
  • (KMTNet Collaboration)
autor
  • Harvard-Smithsonian CfA, 60 Garden St., Cambridge, MA 02138, USA
  • (KMTNet Collaboration)
autor
  • Physics Department and Tsinghua Centre for Astrophysics, Tsinghua University, Beijing 100084, China
  • Department of Physics, Zhejiang University, Hangzhou, 310058, China
  • (KMTNet Collaboration)
autor
  • Canadian Institute for Theoretical Astrophysics, University of Toronto, 60 St George Street, Toronto, ON M5S 3H8, Canada
  • (KMTNet Collaboration)
autor
  • Korea Astronomy and Space Science Institute, Daejon 34055, Korea
  • School of Space Research, Kyung Hee University, Yongin, Kyeonggi 17104, Korea
  • (KMTNet Collaboration)
autor
  • Korea Astronomy and Space Science Institute, Daejon 34055, Korea
  • (KMTNet Collaboration)
autor
  • Korea Astronomy and Space Science Institute, Daejon 34055, Korea
  • (KMTNet Collaboration)
autor
  • Korea Astronomy and Space Science Institute, Daejon 34055, Korea
  • (KMTNet Collaboration)
autor
  • Korea Astronomy and Space Science Institute, Daejon 34055, Korea
  • Korea University of Science and Technology, Daejeon 34113, Korea
  • (KMTNet Collaboration)
autor
  • Korea Astronomy and Space Science Institute, Daejon 34055, Korea
  • (KMTNet Collaboration)
autor
  • Korea Astronomy and Space Science Institute, Daejon 34055, Korea
  • School of Space Research, Kyung Hee University, Yongin, Kyeonggi 17104, Korea
  • (KMTNet Collaboration)
autor
  • Korea Astronomy and Space Science Institute, Daejon 34055, Korea
  • Korea University of Science and Technology, Daejeon 34113, Korea
  • (KMTNet Collaboration)
autor
  • epartment of Astronomy, Ohio State University, 140 W. 18th Ave., Columbus, OH 43210, USA
  • (KMTNet Collaboration)
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Uwagi
Opracowanie rekordu w ramach umowy 509/P-DUN/2018 ze środków MNiSW przeznaczonych na działalność upowszechniającą naukę (2019).
Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-c6c82d39-1952-4087-8666-e178c8557b84
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