Comparative blind test of five planetary transit detection algorithms on realistic synthetic light curves

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作者
Moutou, C. [1 ]
Pont, F. [1 ,5 ]
Barge, P. [1 ]
Aigrain, S. [2 ]
Auvergne, M. [3 ]
Blouin, D. [1 ]
Cautain, R. [1 ]
Erikson, A.R. [6 ]
Guis, V. [1 ]
Guterman, P. [1 ,7 ]
Irwin, M. [2 ]
Lanza, A.F. [4 ]
Queloz, D. [5 ]
Rauer, H. [6 ]
Voss, H. [6 ]
Zucker, S. [5 ,8 ]
机构
[1] LAM, Traverse du Siphon, BP 8, Les Trois Lucs, 13376 Marseille Cedex 12, France
[2] Institute of Astronomy (IoA), University of Cambridge, Madingley Road, Cambridge CB3 0HA, United Kingdom
[3] OPM, Place J. Janssen, 92195 Meudon Cedex, France
[4] INAF, Osservatorio Astrofisico di Catania, via S. Sofia, 78, 95123 Catania, Italy
[5] Observatoire de Genève, 51 Chemin des Maillettes, 1290 Sauverny, Switzerland
[6] DLR Institute of Planetary Research, Rutherfordstr. 2, 12489 Berlin, Germany
[7] Gemplus Card International, La Ciotat, France
[8] Faculty of Physics, Weizman Institute of Science, Rehovot 76100, Israel
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Astronomy and Astrophysics | 1600年 / 437卷 / 01期
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页码:355 / 368
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