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Initial Characteristics of Kepler Short Cadence Data

  • Authors: Ronald L. Gilliland, Jon M. Jenkins, William J. Borucki, Steven T. Bryson, Douglas A. Caldwell, Bruce D. Clarke, Jessie L. Dotson, Michael R. Haas, Jennifer Hall, Todd Klaus, David Koch, Sean McCauliff, Elisa V. Quintana, Joseph D. Twicken, and Jeffrey E. van Cleve

GILLILAND et al. 2010 The Astrophysical Journal Letters 713 L160.

  • Provider: AAS Journals

Caption: Figure 4.

Upper panel shows the 33.5 days of Q1 LC data folded on the ~2.47 day period of TrES-2 with a Kepler magnitude of 11.34. The lower panel shows folded data at SC for the same interval. The curve passing through the points in the upper panel was based on fitting a transit light-curve model integrated over the LC of 29.4 minutes, while for comparison the narrower curve (at top) shows the fit to SC data. The horizontal bar in the upper panel shows the length of an LC interval in phase for TrES-2.

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