A PSF-based approach to Kepler/K2 data – III. Search for exoplanets and variable stars within the open cluster M 67 (NGC 2682)Authors:Nardiello et alAbstract: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.
Friday, December 9, 2016
Search for exoplanets and variable stars within the open cluster M67 (NGC 2682)
Posted by Will Baird at 8:00 AM
Labels: exoplanet detection, kepler, M67, NGC 2682, open cluster, stellar clusters
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