Tytuł artykułu
Autorzy
Udalski A.
Ryu Y.-H.
Sajadian S.
Gould A.
Mróz P.
Poleski R.
Szymański M. K.
Skowron J.
Soszyński I.
Kozłowski S.
Pietrukowicz P.
Ulaczyk K.
Pawlak M.
Rybicki K.
Iwanek P.
Albrow M. D.
Chung S. -J.
Han C.
Hwang K.-H.
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.
Bozza W.
Dominik M.
Helling C.
Hundertmark M.
Jørgensen U. G.
Longa-Peña P.
Lowry S.
Burgdorf M.
Campbell-White J.
Ciceri S.
Evans D.
Jaimes R. F.
Fujii Y. I.
Haikala L. K.
Henning T.
Hinse T. C.
Mancini L.
Peixinho N.
Rahvar S.
Rabus M.
Skottfelt J.
Snodgrass C.
Southworth J.
von Essen C.
Wybrane pełne teksty z tego czasopisma
Identyfikatory
Warianty tytułu
Języki publikacji
Abstrakty
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.
Słowa kluczowe
Czasopismo
Rocznik
Tom
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)
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
- (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)
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,
- (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)
autor
- Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg (ZAH), 69120 Heidelberg, Germany
- (MiNDSTEp Collaboration)
autor
- Niels Bohr Institute & Centre for Star and Planet Formation, University of Copenhagen, Øster Voldgade 5, 1350 Copenhagen, Denmark
- (MiNDSTEp Collaboration)
autor
- 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)
autor
- 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)
autor
- 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)
autor
- 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