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We report the discovery of a cold Super-Earth planet (mp=4.4±0.5 M⊕) orbiting a low-mass (M=0.23±0.03 M⊙) M dwarf at projected separation a=1.18±0.10 a.u., i.e., about 1.9 times the distance the snow line. The system is quite nearby for a microlensing planet, DL=0.86±0.09 kpc. Indeed, it was the large lens-source relative parallax πrel=1.0 mas (combined with the low mass M) that gave rise to the large, and thus well-measured, "microlens parallax" πE∝(πrel/M)1/2 that enabled these precise measurements. OGLE-2017-BLG-1434Lb is the eighth microlensing planet with planet-host mass ratio q<1×10-4. We apply a new planet-detection sensitivity method, which is a variant of "V/Vmax", to seven of these eight planets to derive the mass-ratio function in this regime. We find dN/d lnq ∝ qp, with p=1.05+0.78-0.68, which confirms the "turnover" in the mass function found by Suzuki et al. relative to the power law of opposite sign n=-0.93±0.13 at higher mass ratios q≳2×10-4. We combine our result with that of Suzuki et al. to obtain p=0.73+0.42-0.34.
Czasopismo
Rocznik
Strony
1--42
Opis fizyczny
Bibliogr. 65 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
  • Department of Physics, Isfahan University of Technology, Isfahan 84156-83111, Iran
autor
  • Korea Astronomy and Space Science Institute, Daejon 34055, Korea
  • Max-Planck-Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany
  • Department of Astronomy, Ohio State University, 140 W. 18th Ave., Columbus, OH43210, USA
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, OH43210, USA
  • (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
  • (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
  • (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
  • Department of Physics, Chungbuk National University, Cheongju 28644, RepublicofKorea
  • (KMTNet Collaboration)
autor
  • Korea Astronomy and Space Science Institute, Daejon 34055, 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,
  • (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
  • (KKorea University of Science and Technology, Daejeon 34113, 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
  • Department of Astronomy, Ohio State University, 140 W. 18th Ave., Columbus, OH43210, USA
  • (KMTNet Collaboration)
autor
  • Dipartimento di Fisica "E.R. Caianiello", Università di Salerno, Via Giovanni Paolo II 132, 84084, Fisciano, Italy
  • Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Napoli, Italy
  • (MiNDSTEp Collaboration)
autor
  • Centre for Exoplanet Science, SUPA, School of Physics & Astronomy, University of St Andrews, North Haugh, St Andrews KY16 9SS, UK
  • (MiNDSTEp Collaboration)
autor
  • Centre for Exoplanet Science, SUPA, School of Physics & Astronomy, University of St Andrews, North Haugh, St Andrews KY16 9SS, UK
  • (MiNDSTEp Collaboration)
  • Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg (ZAH), 69120 Heidelberg, Germany
  • (MiNDSTEp Collaboration)
  • Niels Bohr Institute & Centre for Star and Planet Formation, University of Copenhagen, Øster Voldgade 5, 1350 Copenhagen, Denmark
  • (MiNDSTEp Collaboration)
  • Unidad de Astronomìa, Universidad de Antofagasta, Av. Angamos 601, Antofagasta, Chile
  • (MiNDSTEp Collaboration)
autor
  • Centre for Astrophysics & Planetary Science, The University of Kent, Canterbury CT27NH,UK
  • (MiNDSTEp Collaboration)
autor
  • Universität Hamburg, Faculty of Mathematics, Informatics and Natural Sciences, Department of Earth Sciences, Meteorological Institute, Bundesstraße 55, 20146 Hamburg, Germany
  • (MiNDSTEp Collaboration)
  • Centre for Astrophysics & Planetary Science, The University of Kent, Canterbury CT27NH,UK
  • (MiNDSTEp Collaboration)
autor
  • Department of Astronomy, Stockholm University, Alba Nova University Center, 106 91, Stockholm, Sweden
  • (MiNDSTEp Collaboration)
autor
  • Astrophysics Group, Keele University, Staffordshire, ST5 5BG, UK
  • (MiNDSTEp Collaboration)
autor
  • Centre for Exoplanet Science, SUPA, School of Physics & Astronomy, University of St Andrews, North Haugh, St Andrews KY16 9SS, UK
  • (MiNDSTEp Collaboration)
autor
  • Niels Bohr Institute & Centre for Star and Planet Formation, University of Copenhagen, Øster Voldgade 5, 1350 Copenhagen, Denmark
  • Institute for Advanced Research, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, 464-8601, Japan
  • (MiNDSTEp Collaboration)
  • Instituto de Astronomia y Ciencias Planetarias de Atacama, Universidad de Atacama, Copayapu 485, Copiapo, Chile
  • (MiNDSTEp Collaboration)
autor
  • Max-Planck-Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany
  • (MiNDSTEp Collaboration)
autor
  • Korea Astronomy and Space Science Institute, Daejon 34055, Korea
  • (MiNDSTEp Collaboration)
autor
  • Max-Planck-Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany
  • Department of Physics, University of Rome Tor Vergata, Via della Ricerca Scientifica 1, I-00133-Roma, Italy
  • INAF - Astrophysical Observatory of Turin, Via Osservatorio 20, I-10025-Pino Torinese, Italy
  • (MiNDSTEp Collaboration)
autor
  • Unidad de Astronomìa, Universidad de Antofagasta, Av. Angamos 601, Antofagasta, Chile
  • CITEUC - Center for Earth and Space Research of the University of Coimbra, Geophysical and Astronomical Observatory, R. Observatorio s/n, 3040-004 Coimbra, Portugal
  • (MiNDSTEp Collaboration)
autor
  • Department of Physics, Sharif University of Technology, PO Box 11155-9161 Tehran, Iran
  • (MiNDSTEp Collaboration)
autor
  • Instituto de Astrofisica, Pontificia Universidad Católica de Chile, Av. Vicuña Mackenna 4860, 7820436 Macul, Santiago, Chile
  • Korea University of Science and Technology, Daejeon 34113, Korea
  • (MiNDSTEp Collaboration)
autor
  • Centre for Electronic Imaging, Department of Physical Sciences, The Open University, Milton Keynes, MK7 6AA, UK
  • (MiNDSTEp Collaboration)
autor
  • School of Physical Sciences, Faculty of Science, Technology, Engineering and Mathematics, The Open University, Walton Hall, Milton Keynes, MK7 6AA, UK
  • (MiNDSTEp Collaboration)
  • Astrophysics Group, Keele University, Staffordshire, ST5 5BG, UK
  • (MiNDSTEp Collaboration)
autor
  • Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, 8000 Aarhus C, Denmark
  • (MiNDSTEp 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-c46bc590-b8b9-42f1-81d4-bdad09a7c07c
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