Planetary systems; Stars: fundamental parameters; Techniques: photometric; Astronomy; Accurate measurement; Contact points; Jupiters; Physical parameters; Planetary system; Stars:fundamental parameters; Photometry
Abstract :
[en] Context. The extrasolar planet WASP-67 b is the first hot Jupiter definitively known to undergo only partial eclipses. The lack of the second and third contact points in this planetary system makes it difficult to obtain accurate measurements of its physical parameters.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Mancini, L.; Max-Planck Institute for Astronomy, Königstuhl 17, Heidelberg, Germany
Southworth, J.; Astrophysics Group, Keele University, Staffordshire, United Kingdom
Ciceri, S.; Max-Planck Institute for Astronomy, Königstuhl 17, Heidelberg, Germany
Calchi Novati, S.; International Institute for Advanced Scientific Studies (IIASS), Vietri Sul Mare (SA), Italy, Department of Physics, University of Salerno, Via Giovanni Paolo II, Fisciano, Italy
Dominik, M.; SUPA, University of St Andrews, School of Physics and Astronomy, North-Haugh, St-Andrews, United Kingdom
Henning, Th; Max-Planck Institute for Astronomy, Königstuhl 17, Heidelberg, Germany
Jørgensen, U. G.; Niels Bohr Institute, University of Copenhagen, Juliane Maries vej 30, Copenhagen Ø, Denmark, Centre for Star and Planet Formation, Geological Museum, Øster Voldgade 5-7, Copenhagen, Denmark
Korhonen, H.; Niels Bohr Institute, University of Copenhagen, Juliane Maries vej 30, Copenhagen Ø, Denmark, Centre for Star and Planet Formation, Geological Museum, Øster Voldgade 5-7, Copenhagen, Denmark, Finnish Centre for Astronomy with ESO (FINCA), University of Turku, Väisäläntie 20, Piikkiö, Finland
Nikolov, N.; Astrophysics Group, University of Exeter, Stocker Road, Exeter, United Kingdom
Alsubai, K. A.; Qatar Foundation, PO Box 5825, Doha, Qatar
Bozza, V.; Department of Physics, University of Salerno, Via Giovanni Paolo II, Fisciano, Italy, Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Napoli, Napoli, Italy
Bramich, D. M.; Qatar Environment and Energy Research Institute, Qatar Foundation, Tornado Tower, PO Box 5825, Doha, Qatar
D'Ago, G.; Department of Physics, University of Salerno, Via Giovanni Paolo II, Fisciano, Italy, Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Napoli, Napoli, Italy
Figuera Jaimes, R.; SUPA, University of St Andrews, School of Physics and Astronomy, North-Haugh, St-Andrews, United Kingdom, European Southern Observatory, Karl-Schwarzschild-Straße 2, Garching bei München, Germany
Galianni, P.; SUPA, University of St Andrews, School of Physics and Astronomy, North-Haugh, St-Andrews, United Kingdom
Gu, S.-H.; Yunnan Observatories, Chinese Academy of Sciences, Kunming, China, Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming, China
Harpsøe, K.; Niels Bohr Institute, University of Copenhagen, Juliane Maries vej 30, Copenhagen Ø, Denmark, Centre for Star and Planet Formation, Geological Museum, Øster Voldgade 5-7, Copenhagen, Denmark
Hinse, T. C.; Korea Astronomy and Space Science Institute, Daejeon, South Korea
Hundertmark, M.; SUPA, University of St Andrews, School of Physics and Astronomy, North-Haugh, St-Andrews, United Kingdom
Juncher, D.; Niels Bohr Institute, University of Copenhagen, Juliane Maries vej 30, Copenhagen Ø, Denmark, Centre for Star and Planet Formation, Geological Museum, Øster Voldgade 5-7, Copenhagen, Denmark
Kains, N.; Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD, United States
Popovas, A.; Niels Bohr Institute, University of Copenhagen, Juliane Maries vej 30, Copenhagen Ø, Denmark, Centre for Star and Planet Formation, Geological Museum, Øster Voldgade 5-7, Copenhagen, Denmark
Rabus, M.; Max-Planck Institute for Astronomy, Königstuhl 17, Heidelberg, Germany, Instituto de Astrofísica, Facultad de Física, Pontificia Universidad Católica de Chile, Av. Vicuña Mackenna 4860, Macul, Santiago, Chile
Rahvar, S.; Department of Physics, Sharif University of Technology, PO Box 11155-9161, Tehran, Iran
Skottfelt, J.; Niels Bohr Institute, University of Copenhagen, Juliane Maries vej 30, Copenhagen Ø, Denmark, Centre for Star and Planet Formation, Geological Museum, Øster Voldgade 5-7, Copenhagen, Denmark
Snodgrass, C.; Max Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, Göttingen, Germany
Street, R.; Las Cumbres Observatory Global Telescope Network, 6740B Cortona Drive, Goleta, CA, United States
Surdej, Jean ; Université de Liège > Département d'astrophys., géophysique et océanographie (AGO) > Astroph. extragalactique et observations spatiales (AEOS)
Tsapras, Y.; Las Cumbres Observatory Global Telescope Network, 6740B Cortona Drive, Goleta, CA, United States, School of Physics and Astronomy, Queen Mary University of London, Mile End Road, London, E1 4NS, United Kingdom
Vilela, C.; Astrophysics Group, Keele University, Staffordshire, United Kingdom
Wang, X.-B.; Yunnan Observatories, Chinese Academy of Sciences, Kunming, China, Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming, China
Wertz, Olivier ; Université de Liège > Département d'astrophys., géophysique et océanographie (AGO) > Astroph. extragalactique et observations spatiales (AEOS)
