activity
20092024
most citedThe K2 Mission: Characterization and Early results

1.7k citations · 22.3k across the 180 of their papers we have counts for

collaborators
Showing 2013Show all

19 papers · 1 filter

astro-ph.EP2013★ 231 cited

Planetary Candidates Observed by Kepler IV: Planet Sample From Q1-Q8 (22 Months)

Christopher J. Burke, Stephen T. Bryson, F. Mullally +37

We provide updates to the Kepler planet candidate sample based upon nearly two years of high-precision photometry (i.e., Q1-Q8). From an initial list of nearly 13,400 Threshold Cro…

astro-ph.SR2013★ 46 cited

KIC11911480: the second ZZ Ceti in the field

S. Greiss, B. T. Gaensicke, J. J. Hermes +5

We report the discovery of the second pulsating hydrogen-rich (DA) white dwarf in the field, KIC11911480. It was selected from the -INT Survey (KIS) on the basis o…

astro-ph.GA2013★ 9 cited

BOKS 45906: a CV with an orbital period of 56.6 min in the Kepler field?

Gavin Ramsay, Steve B. Howell, Matt A. Wood +6

BOKS 45906 was found to be a blue source in the Burrell-Optical-Kepler-Survey which showed a 3 mag outburst lasting ~5 d. We present the Kepler light curve of this source which cov…

astro-ph.EP2013★ 39 cited

Detection of Potential Transit Signals in Sixteen Quarters of Kepler Mission Data

Peter Tenenbaum, Jon M. Jenkins, Shawn Seader +25

We present the results of a search for potential transit signals in four years of photometry data acquired by the Kepler Mission. The targets of the search include 111,800 stars wh…

astro-ph.SR2013★ 40 cited

RATS-Kepler -- a deep high cadence survey of the Kepler field

Gavin Ramsay, Adam Brooks, Pasi Hakala +8

We outline the purpose, strategy and first results of a deep, high cadence, photometric survey of the Kepler field using the Isaac Newton Telescope on La Palma and the MDM 1.3m Tel…

astro-ph.EP2013★ 290 cited

Inference of Inhomogeneous Clouds in an Exoplanet Atmosphere

Brice-Olivier Demory, Julien de Wit, Nikole Lewis +11

We present new visible and infrared observations of the hot Jupiter Kepler-7b to determine its atmospheric properties. Our analysis allows us to 1) refine Kepler-7b's relatively la…