Bibcode
Erikson, A.; Santerne, A.; Renner, S.; Barge, P.; Aigrain, S.; Alapini, A.; Almenara, J.-M.; Alonso, R.; Auvergne, M.; Baglin, A.; Benz, W.; Bonomo, A. S.; Borde, P.; Bouchy, F.; Bruntt, H.; Cabrera, J.; Carone, L.; Carpano, S.; Csizmadia, Sz.; Deleuil, M.; Deeg, H. J.; Diaz, R. F.; Dvorak, R.; Ferraz-Mello, S.; Fridlund, M.; Gandolfi, D.; Gazzano, J.-C.; Gillon, M.; Guenther, E. W.; Guillot, T.; Hatzes, A.; Hebrard, G.; Jorda, L.; Lammer, H.; Leger, A.; Llebaria, A.; Mayor, M.; Mazeh, T.; Moutou, C.; Ollivier, M.; Ofir, A.; Paetzold, M.; Pepe, F.; Pont, F.; Queloz, D.; Rabus, M.; Rauer, H.; Regulo, C.; Rouan, D.; Samuel, B.; Schneider, J.; Shporer, A.; Tingley, B.; Udry, S.; Wuchterl, G.
Bibliographical reference
VizieR On-line Data Catalog: J/A+A/539/A14. Originally published in: 2012A&A...539A..14E
Advertised on:
4
2012
Citations
0
Refereed citations
0
Description
Among the acquired data, we analyzed those for 1269 sources in the
chromatic bands and 5705 in the monochromatic band. Instrumental noise
and the stellar variability were treated with several detrending tools,
to which several transit-search algorithms were subsequently applied.
Fifty-one sources were classified as planetary transit candidates and 26
were followed up with ground-based observations. Until now, no planet
has been detected in the CoRoT data from the SRc01 field.
(1 data file).