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.; Bordé, P.; Bouchy, F.; Bruntt, H.; Cabrera, J.; Carone, L.; Carpano, S.; Csizmadia, Sz.; Deleuil, M.; Deeg, H. J.; Díaz, R. F.; Dvorak, R.; Ferraz-Mello, S.; Fridlund, M.; Gandolfi, D.; Gazzano, J.-C.; Gillon, M.; Guenther, E. W.; Guillot, T.; Hatzes, A.; Hébrard, G.; Jorda, L.; Lammer, H.; Léger, A.; Llebaria, A.; Mayor, M.; Mazeh, T.; Moutou, C.; Ollivier, M.; Ofir, A.; Pätzold, M.; Pepe, F.; Pont, F.; Queloz, D.; Rabus, M.; Rauer, H.; Régulo, C.; Rouan, D.; Samuel, B.; Schneider, J.; Shporer, A.; Tingley, B.; Udry, S.; Wuchterl, G.
Referencia bibliográfica
Astronomy and Astrophysics, Volume 539, id.A14
Fecha de publicación:
3
2012
Revista
Número de citas
23
Número de citas referidas
20
Descripción
Context. The space mission CoRoT is devoted to the analysis of stellar
variability and the photometric detection of extrasolar planets.
Aims: We present the list of planetary transit candidates detected in
the first short run observed by CoRoT that targeted SRc01, towards the
Galactic center in the direction of Aquila, which lasted from April to
May 2007. Methods: 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. Results: 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.
The CoRoT space mission, launched on December 27th 2006, has been
developed and is operated by CNES, with contributions from Austria,
Belgium, Brazil, ESA, Germany, and Spain. The CoRoT data are available
to the community from the CoRoT archive: http://idoc-corot.ias.u-psud.frBased
in part on observations made with the 1.93-m telescope at Observatoire
de Haute Provence (CNRS), France (SOPHIE Program 08A.PNP.MOUT).Based in
part on observations made with the ESO-3.60-m telescope at La Silla
Observatory (ESO), Chile (HARPS Program ESO - 081.C-0388) and with the
ESO-VLT telescope at Paranal Observatory (ESO), Chile (FLAMES Program
ESO - 081.C-0413).
Proyectos relacionados
Sismología Solar y Estelar y Búsqueda de Exoplanetas
Los objetivos genéricos de este Proyecto son: 1) el estudio de la estructura y dinámica del interior solar, 2) la extensión de dicho estudio al caso de otras estrellas, 3) la búsqueda y caracterización de planetas extrasolares por métodos fotométricos (principalmente mediante el método de tránsitos) y espectroscópico (variaciones en la velocidad
Savita
Mathur