The secondary eclipse of CoRoT-1b

The transiting planet CoRoT-1b is thought to belong to the pM-class of planets, in which the thermal emission dominates in the optical wavelengths. We present a detection of its secondary eclipse in the CoRoT white channel data, whose response function goes from ~400 to ~1000 nm. We used two differe...

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Bibliographic Details
Main Authors:	Alonso, R, Alapini, A, Aigrain, S, Auvergne, M, Baglin, A, Barbieri, M, Barge, P, Bonomo, A, Borde, P, Bouchy, F, Chaintreuil, S, Reza, R, Deeg, H, Deleuil, M, Dvorak, R, Erikson, A, Fridlund, M, Fialho, F, Gondoin, P, Guillot, T, Hatzes, A, Jorda, L, Lammer, H, Leger, A, Llebaria, A
Format:	Journal article
Language:	English
Published:	2009

The secondary eclipse of CoRoT-1b

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