Fig. 5
High-resolution SDSSi images of the close companions detected around 3 arcsec of the 17 Kepler objects of interest. North towards up and east towards left. Different sizes are used for each image to clearly show all features. Black arrows indicate the position of the faintest targets and the horizontal black line represents 2 arcsec on each image. Green polygons represent the optimal public Kepler apertures used on each quarter of the Kepler mission to compute the light curves.The brighter object assumed to be the KOI is centered on the images for reconnaissance purposes.
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