Characteristics of Kepler Planetary Candidates Based on the First Data Set
In the spring of 2009, the Kepler Mission commenced high-precision photometry on nearly 156,000 stars to determine the frequency and characteristics of small exoplanets, conduct a guest observer program, and obtain asteroseismic data on a wide variety of stars. On 2010 June 15, the Kepler Mission re...
Main Author: | Seager, Sara |
---|---|
Other Authors: | Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences |
Format: | Article |
Language: | en_US |
Published: |
IOP Publishing
2012
|
Online Access: | http://hdl.handle.net/1721.1/74157 https://orcid.org/0000-0002-6892-6948 |
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