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Kepler (microarchitecture)

Known as: Kepler (disambiguation), Kepler architecture, Nvidia Kepler Architecture 
Kepler is the codename for a GPU microarchitecture developed by Nvidia as the successor to the Fermi microarchitecture. Kepler is Nvidia's first… 
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Papers overview

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Highly Cited
2015
Highly Cited
2015
CORRELATIONS BETWEEN COMPOSITIONS AND ORBITS ESTABLISHED BY THE GIANT IMPACT ERA OF PLANET FORMATION
The giant impact phase of terrestrial planet formation establishes connections between super-Earths’ orbital properties… 
Highly Cited
2015
Highly Cited
2015
THE KEPLER DICHOTOMY IN PLANETARY DISKS: LINKING KEPLER OBSERVABLES TO SIMULATIONS OF LATE-STAGE PLANET FORMATION
NASA’s Kepler Mission uncovered a wealth of planetary systems, many with planets on short-period orbits. These short-period… 
Highly Cited
2014
Highly Cited
2014
MOST SUB-ARCSECOND COMPANIONS OF KEPLER EXOPLANET CANDIDATE HOST STARS ARE GRAVITATIONALLY BOUND
Using the known detection limits for high-resolution imaging observations and the statistical properties of true binary and line… 
Review
2014
Review
2014
PLANETESIMAL INTERACTIONS CAN EXPLAIN THE MYSTERIOUS PERIOD RATIOS OF SMALL NEAR-RESONANT PLANETS
An intriguing trend among Kepler’s multi-planet systems is an overabundance of planet pairs with period ratios just wide of a… 
Highly Cited
2014
Highly Cited
2014
CHARACTERIZING K2 PLANET DISCOVERIES: A SUPER-EARTH TRANSITING THE BRIGHT K DWARF HIP 116454
We report the first planet discovery from the two-wheeled Kepler (K2) mission: HIP 116454 b. The host star HIP 116454 is a bright… 
Review
2013
Review
2013
ASTEROSEISMIC CLASSIFICATION OF STELLAR POPULATIONS AMONG 13,000 RED GIANTS OBSERVED BY KEPLER
Of the more than 150,000 targets followed by the Kepler Mission, about 10% were selected as red giants. Due to their high… 
Highly Cited
2013
Highly Cited
2013
TESTING IN SITU ASSEMBLY WITH THE KEPLER PLANET CANDIDATE SAMPLE
We present a Monte Carlo model for the structure of low-mass (total mass <25 M⊕) planetary systems that form by the in situ… 
Highly Cited
2012
Highly Cited
2012
THE ORIGIN OF KEPLER'S SUPERNOVA REMNANT
It is now well established that Kepler's supernova remnant (SNR) is the result of a Type Ia explosion. With an age of 407 yr and… 
2011
2011
AT LAST—A V777 HER PULSATOR IN THE KEPLER FIELD
We present the discovery of the first—and so far the only—pulsating white dwarf star located in the field of view of the Kepler… 
Highly Cited
2003
Highly Cited
2003
Efficient Orbit Integration by Scaling for Kepler Energy Consistency
Extending Nacozy's idea of manifold correction by using the concept of the integral invariant relation, we propose a new approach… 
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