Tytuł artykułu
Autorzy
Skowron J.
Ryu Y.-H.
Hwang K.-H.
Udalski A.
Mróz P.
Kozłowski S.
Soszyński I.
Pietrukowicz P.
Szymański M. K.
Poleski R.
Ulaczyk K.
Pawlak M.
Rybicki K.
Iwanek P.
Albrow M. D.
Chung S.-J.
Gould A.
Han C.
Jung Y. K.
Shin I.-G.
Shvartzvald Y.
Yee J. C.
Zang W.
Zhu W.
Cha S.-M.
Kim D.-J.
Kim H.-W.
Kim S.-L.
Lee C.-U.
Lee D.-J
Lee Y.
Park B.-G.
Pogge R. W.
Wybrane pełne teksty z tego czasopisma
Identyfikatory
Warianty tytułu
Języki publikacji
Abstrakty
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.
Słowa kluczowe
Czasopismo
Rocznik
Tom
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)
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
- 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)
autor
- 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)
Bibliografia
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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