Full Content is available to subscribers

Subscribe/Learn More  >
Proceedings Article

Kepler instrument performance: an in-flight update

[+] Author Affiliations
Douglas A. Caldwell, Jeffrey E. Van Cleve, Jon M. Jenkins, Peter Tenenbaum, Jie Li, Hayley Wu

NASA Ames Research Ctr. (USA)

Vic S. Argabright

Ball Aerospace & Technologies Corp. (USA)

Jeffery J. Kolodziejczak

NASA Marshall Space Flight Ctr. (USA)

Edward W. Dunham

Lowell Observatory (USA)

John C. Geary

Smithsonian Astrophysical Observatory (USA)

Hema Chandrasekaran

NASA Ames Research Ctr. (USA) and Lawrence Livermore National Lab. (USA)

Jason Von Wilpert

Univ. of California, Santa Cruz (USA)

Proc. SPIE 7731, Space Telescopes and Instrumentation 2010: Optical, Infrared, and Millimeter Wave, 773117 (August 05, 2010); doi:10.1117/12.856638
Text Size: A A A
From Conference Volume 7731

  • Space Telescopes and Instrumentation 2010: Optical, Infrared, and Millimeter Wave
  • Jacobus M. Oschmann, Jr.; Mark C. Clampin; Howard A. MacEwen
  • San Diego, California, USA | June 27, 2010


The Kepler Mission is designed to detect the 80 parts per million (ppm) signal from an Earth-Sun equivalent transit. Such precision requires superb instrument stability on time scales up to 2 days and systematic error removal to better than 20 ppm. The sole scientific instrument is the Photometer, a 0.95 m aperture Schmidt telescope that feeds the 94.6 million pixel CCD detector array, which contains both Science and Fine Guidance Sensor (FGS) CCDs. Since Kepler's launch in March 2009, we have been using the commissioning and science operations data to characterize the instrument and monitor its performance. We find that the in-flight detector properties of the focal plane, including bias levels, read noise, gain, linearity, saturation, FGS to Science crosstalk, and video crosstalk between Science CCDs, are essentially unchanged from their pre-launch values. Kepler's unprecedented sensitivity and stability in space have allowed us to measure both short- and long- term effects from cosmic rays, see interactions of previously known image artifacts with starlight, and uncover several unexpected systematics that affect photometric precision. Based on these results, we expect to attain Kepler's planned photometric precision over 90% of the field of view.

© (2010) COPYRIGHT SPIE--The International Society for Optical Engineering. Downloading of the abstract is permitted for personal use only.

Douglas A. Caldwell ; Jeffrey E. Van Cleve ; Jon M. Jenkins ; Vic S. Argabright ; Jeffery J. Kolodziejczak, et al.
"Kepler instrument performance: an in-flight update", Proc. SPIE 7731, Space Telescopes and Instrumentation 2010: Optical, Infrared, and Millimeter Wave, 773117 (August 05, 2010); doi:10.1117/12.856638; http://dx.doi.org/10.1117/12.856638

Access This Article
Sign In to Access Full Content
Please Wait... Processing your request... Please Wait.
Sign in or Create a personal account to Buy this article ($15 for members, $18 for non-members).



Citing articles are presented as examples only. In non-demo SCM6 implementation, integration with CrossRef’s "Cited By" API will populate this tab (http://www.crossref.org/citedby.html).

Some tools below are only available to our subscribers or users with an online account.

Related Content

Customize your page view by dragging & repositioning the boxes below.

Related Book Chapters

Topic Collections


Buy this article ($18 for members, $25 for non-members).
Sign In