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20042022
most citedKepler Mission Design, Realized Photometric Performance, and Early Science

1.2k citations · 6.9k across the 51 of their papers we have counts for

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Showing 2010Show all

7 papers · 1 filter

astro-ph.EP2010★ 355 cited

Characteristics of Kepler Planetary Candidates Based on the First Data Set: The Majority are Found to be Neptune-Size and Smaller

William J. Borucki

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…

astro-ph.SR2010★ 7 cited

Solar-like oscillations in cluster stars

D. Stello, S. Basu, T. R. Bedding +21

We present a brief overview of the history of attempts to obtain a clear detection of solar-like oscillations in cluster stars, and discuss the results on the first clear detection…

astro-ph.EP2010★ 1.2k cited

Kepler Mission Design, Realized Photometric Performance, and Early Science

David G. Koch, William J. Borucki, Gibor Basri +44

The Kepler Mission, launched on Mar 6, 2009 was designed with the explicit capability to detect Earth-size planets in the habitable zone of solar-like stars using the transit photo…

astro-ph.EP2010★ 111 cited

Discovery and Rossiter-McLaughlin Effect of Exoplanet Kepler-8b

Jon M. Jenkins, William J. Borucki, David G. Koch +50

We report the discovery and the Rossiter-McLaughlin effect of Kepler-8b, a transiting planet identified by the NASA Kepler Mission. Kepler photometry and Keck-HIRES radial velociti…

astro-ph.SR2010★ 151 cited

Photometric Variability in Kepler Target Stars: The Sun Among Stars -- A First Look

Gibor Basri, Lucianne M. Walkowicz, Natalie Batalha +10

The Kepler mission provides an exciting opportunity to study the lightcurves of stars with unprecedented precision and continuity of coverage. This is the first look at a large sam…

astro-ph.SR2010★ 313 cited

Selection, Prioritization, and Characteristics of Kepler Target Stars

N. M. Batalha, W. J. Borucki, D. G. Koch +8

The Kepler Mission began its 3.5-year photometric monitoring campaign in May 2009 on a select group of approximately 150,000 stars. The stars were chosen from the ~half million in…