CoRoT-10b: a giant planet in a 13.24 day eccentric orbit

(2010)

Authors:

AS Bonomo, A Santerne, R Alonso, J-C Gazzano, M Havel, S Aigrain, M Auvergne, A Baglin, M Barbieri, P Barge, W Benz, P Bordé, F Bouchy, H Bruntt, J Cabrera, AC Cameron, L Carone, S Carpano, Sz Csizmadia, M Deleuil, HJ Deeg, R Dvorak, A Erikson, S Ferraz-Mello, M Fridlund, D Gandolfi, M Gillon, E Guenther, T Guillot, A Hatzes, G Hébrard, L Jorda, H Lammer, AF Lanza, A Léger, A Llebaria, M Mayor, T Mazeh, C Moutou, M Ollivier, M Pätzold, F Pepe, D Queloz, H Rauer, D Rouan, B Samuel, J Schneider, B Tingley, S Udry, G Wuchterl

Accretion dynamics and disk evolution in NGC 2264: a study based on the Corot photometric observations

(2010)

Authors:

SHP Alencar, PS Teixeira, MM Guimaraes, PT McGinnis, JF Gameiro, J Bouvier, S Aigrain, E Flaccomio, F Favata

Photospheric activity, rotation, and radial velocity variations of the planet-hosting star CoRoT-7

(2010)

Authors:

AF Lanza, AS Bonomo, C Moutou, I Pagano, S Messina, G Leto, G Cutispoto, S Aigrain, R Alonso, P Barge, M Deleuil, M Auvergne, A Baglin, A Collier Cameron

The SARS algorithm: Detrending CoRoT light curves with Sysrem using simultaneous external parameters

Monthly Notices of the Royal Astronomical Society: Letters 404:1 (2010)

Authors:

A Ofir, R Alonso, AS Bonomo, L Carone, S Carpano, B Samuel, J Weingrill, S Aigrain, M Auvergne, A Baglin, P Barge, P Borde, F Bouchy, HJ Deeg, M Deleuil, R Dvorak, A Erikson, SF Mello, M Fridlund, M Gillon, T Guillot, A Hatzes, L Jorda, H Lammer, A Leger, A Llebaria, C Moutou, M Ollivier, M Päetzold, D Queloz, H Rauer, D Rouan, J Schneider, G Wuchterl

Abstract:

Surveys for exoplanetary transits are usually limited not by photon noise but rather by the amount of red noise in their data. In particular, although the CoRoT space-based survey data are being carefully scrutinized, significant new sources of systematic noises are still being discovered. Recently, a magnitude-dependant systematic effect was discovered in the CoRoT data by Mazeh et al. and a phenomenological correction was proposed. Here we tie the observed effect to a particular type of effect, and in the process generalize the popular Sysrem algorithm to include external parameters in a simultaneous solution with the unknown effects. We show that a post-processing scheme based on this algorithm performs well and indeed allows for the detection of new transit-like signals that were not previously detected. © 2010 The Authors. Journal compilation © 2010 RAS.

Ground-based detection of thermal emission from the exoplanet WASP-19b

\mnras 404 (2010) L114-L118-L114-L118

Authors:

NP Gibson, S Aigrain, DL Pollacco, SCC Barros, L Hebb, M Hrudková, EK Simpson, I Skillen, R West