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机译:完全确定的微透镜观测策略的推论实现† sup>
Niels Bohr Institutet, Københavns Universitet, Juliane Maries Vej 30, 2100 København Ø, Denmark|Centre for Star and Planet Formation, Københavns Universitet, Øster Voldgade 5-7, 1350 København Ø, Denmark;
Department of Physics, The University of Auckland, Private Bag 92019, New Zealand;
Niels Bohr Institutet, Københavns Universitet, Juliane Maries Vej 30, 2100 København Ø, Denmark;
Niels Bohr Institutet, Københavns Universitet, Juliane Maries Vej 30, 2100 København Ø, Denmark|Armagh Observatory, College Hill, Armagh, BT61 9DG, UK;
Universitdegli Studi di Salerno, Dipartimento di Fisica “E.R. Caianiello”, Via Ponte Don Melillo, 84085 Fisciano (SA), Italy|INFN, Gruppo Collegato di Salerno, Sezione di Napoli, Italy|Istituto Internazionale per gli Alti Studi Scientifici (IIASS), Via G. Pellegrino 19, 84019 Vietri sul Mare (SA), Italy;
Niels Bohr Institutet, Københavns Universitet, Juliane Maries Vej 30, 2100 København Ø, Denmark;
Universitdegli Studi di Salerno, Dipartimento di Fisica “E.R. Caianiello”, Via Ponte Don Melillo, 84085 Fisciano (SA), Italy|INFN, Gruppo Collegato di Salerno, Sezione di Napoli, Italy|Istituto Internazionale per gli Alti Studi Scientifici (IIASS), Via G. Pellegrino 19, 84019 Vietri sul Mare (SA), Italy;
Astronomisches Rechen-Institut, Zentrum für Astronomie der Universitt Heidelberg (ZAH), Mönchhofstr. 12-14, 69120 Heidelberg, Germany|Departamento de Astronomía y Astrofísica, Pontificia Universidad Católica de Chile, Vicuña Mackenna 4860, 7820436 Macul, Santiago, Chile;
Deutsches SOFIA Institut, Universitt Stuttgart, Pfaffenwaldring 31, 70569 Stuttgart, Germany|SOFIA Science Center, NASA Ames Research Center, Mail Stop N211-3, Moffett Field CA 94035, USA;
SUPA, University of St Andrews, School of Physics & Astronomy, North Haugh, St Andrews, KY16 9SS, UK;
Institut für Astrophysik, Georg-August-Universitt, Friedrich-Hund-Platz 1, 37077 Göttingen, Germany;
Jodrell Bank Centre for Astrophysics, University of Manchester, Alan Turing Building, Manchester, M13 9PL, UK;
Niels Bohr Institutet, Københavns Universitet, Juliane Maries Vej 30, 2100 København Ø, Denmark;
SUPA, University of St Andrews, School of Physics & Astronomy, North Haugh, St Andrews, KY16 9SS, UK|Astronomisches Rechen-Institut, Zentrum für Astronomie der Universitt Heidelberg (ZAH), Mönchhofstr. 12-14, 69120 Heidelberg, Germany;
Universitdegli Studi di Salerno, Dipartimento di Fisica “E.R. Caianiello”, Via Ponte Don Melillo, 84085 Fisciano (SA), Italy|INFN, Gruppo Collegato di Salerno, Sezione di Napoli, Italy|Istituto Internazionale per gli Alti Studi Scientifici (IIASS), Via G. Pellegrino 19, 84019 Vietri sul Mare (SA), Italy|Dipartimento di Ingegneria, Universitdel Sannio, Corso Garibaldi 107, 82100 Benevento, Italy;
Bellatrix Astronomical Observatory, Via Madonna de Loco 47, 03023 Ceccano (FR), Italy;
Department of Physics, Sharif University of Technology, P. O. Box 11155–9161, Tehran, Iran;
Institut d'Astrophysique et de Géophysique, Allée du 6 Aoüt 17, Sart Tilman, Bât. B5c, 4000 Liège, Belgium;
Universitdegli Studi di Salerno, Dipartimento di Fisica “E.R. Caianiello”, Via Ponte Don Melillo, 84085 Fisciano (SA), Italy|INFN, Gruppo Collegato di Salerno, Sezione di Napoli, Italy|Istituto Internazionale per gli Alti Studi Scientifici (IIASS), Via G. Pellegrino 19, 84019 Vietri sul Mare (SA), Italy;
Max Planck Institute for Solar System Research, Max-Planck-Str. 2, 37191 Katlenburg-Lindau, Germany|European Southern Observatory, Alonso de Cordova 3107, Casilla 19001, Santiago 19, Chile;
Astrophysics Group, Keele University, Staffordshire, ST5 5BG, UK;
Las Cumbres Observatory Global Telescope Network, 6740B Cortona Dr, Goleta, CA 93117, USA;
Institut d'Astrophysique et de Géophysique, Allée du 6 Aoüt 17, Sart Tilman, Bât. B5c, 4000 Liège, Belgium;
Niels Bohr Institutet, Københavns Universitet, Juliane Maries Vej 30, 2100 København Ø, Denmark|INAF, Osservatorio Astronomico di Brera, 23807 Merate (LC), Italy;
Las Cumbres Observatory Global Telescope Network, 6740B Cortona Dr, Goleta, CA 93117, USA|School of Mathematical Sciences, Queen Mary, University of London, London, E1 4NS, UK;
Astronomisches Rechen-Institut, Zentrum für Astronomie der Universitt Heidelberg (ZAH), Mönchhofstr. 12-14, 69120 Heidelberg, Germany;
Astronomisches Rechen-Institut, Zentrum für Astronomie der Universitt Heidelberg (ZAH), Mönchhofstr. 12-14, 69120 Heidelberg, Germany;
gravitational lensing; planetary systems;
机译:实现用于确定行星总数的全确定性微透镜观测策略
机译:韩国微透镜电视网络的最佳调查策略和预计的单产
机译:引力微透镜行星搜索的两种后续观察策略的比较
机译:微溶剂搜索额外行星:观察战略,发现和中度专用
机译:引力微透镜发现的行星的直接质量测量和光曲线建模
机译:从宿主恒星金属性推断出三种太阳系外行星半径
机译:实现用于确定行星总数的全确定性微透镜观测策略
机译:观察行星轴承磁盘和磁盘嵌入行星