Direct measurement of the Kepler Space Telescope CCD's intra-pixel response function

26 Sep 2019 Vorobiev Dmitry Irwin Alexis Ninkov Zoran Donlon Kevan Caldwell Douglas Mochnacki Stefan

Space missions designed for high precision photometric monitoring of stars often under-sample the point-spread function, with much of the light landing within a single pixel. Missions like MOST, Kepler, BRITE, and TESS, do this to avoid uncertainties due to pixel-to-pixel response nonuniformity... (read more)

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  • INSTRUMENTATION AND METHODS FOR ASTROPHYSICS