2016/08/26 by D. Nardiello, M. Libralato, Mattia Libralato +6 · 1 citation
Physics and Astronomy · #Asteroseismology #Astro and Planetary Science #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Exoplanet #Kepler #Light curve #Metallicity #Open cluster #Physics #Planet #Planetary system #Stars #Stellar, planetary, and galactic studies #Variable star #astro-ph.EP #astro-ph.IM #astro-ph.SR
paper · pdf · doi:10.1093/mnras/stw2169
14 pages, 9 figures (1 at low resolution), 3 tables. Accepted for publication in MNRAS on August 24, 2016. Electronic materials are available at http://groups.dfa.unipd.it/ESPG/Kepler-K2.html
openalex publication_date 2016/08/26 · arxiv created 2016/08/30 · arxiv updated 2016/09/07 · openalex created_date 2016/09/16 · openalex updated_date 2026/08/05
In the third paper of this series we continue the exploitation of Kepler/K2 data in dense stellar fields using our PSF-based method. This work is focused on a ∼720-arcmin2 region centred on the Solar-metallicity and Solar-age open cluster M 67. We extracted light curves for all detectable sources in the Kepler channels 13 and 14, adopting our technique based on the usage of a high-angular-resolution input catalogue and target-neighbour subtraction. We detrended light curves for systematic errors, and searched for variables and exoplanets using several tools. We found 451 variables, of which 299 are new detection. Three planetary candidates were detected by our pipeline in this field. Raw and detrended light curves, catalogues, and K2 stacked images used in this work will be released to the community.