Volume 594, October 2016
|Number of page(s)||9|
|Section||Catalogs and data|
|Published online||19 October 2016|
New planetary and eclipsing binary candidates from campaigns 1−6 of the K2 mission⋆
1 Instituto de Astrofísica e Ciências
do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, PT, 4150-762 Porto, Portugal
2 Aix Marseille Université, CNRS, LAM (Laboratoire d’Astrophysique de Marseille) UMR 7326, 13388 Marseille, France
Accepted: 7 July 2016
Context. With only two functional reaction wheels, Kepler cannot maintain stable pointing at its original target field and has entered a new mode of observation called K2.
Aims. We describe a new pipeline to reduce K2 pixel files into light curves that are later searched for transit like features.
Methods. Our method is based on many years of experience in planet hunting for the CoRoT mission. Owing to the unstable pointing, K2 light curves present systematics that are correlated with the target position in the charge coupled device (CCD). Therefore, our pipeline also includes a decorrelation of this systematic noise. Our pipeline is optimised for bright stars for which spectroscopic follow-up is possible. We achieve a maximum precision on 6 hours of 6 ppm. The decorrelated light curves are searched for transits with an adapted version of the CoRoT alarm pipeline.
Results. We present 172 planetary candidates and 327 eclipsing binary candidates from campaigns 1, 2, 3, 4, 5, and 6 of K2. Both the planetary candidates and eclipsing binary candidates lists are made public to promote follow-up studies. The light curves will also be available to the community.
Key words: planets and satellites: detection / binaries: eclipsing / techniques: photometric
Full Tables A.1 and A.2 are only available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (188.8.131.52) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/594/A100
© ESO 2016
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