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Kepler (microarchitecture)
Known as:
Kepler (disambiguation)
, Kepler architecture
, Nvidia Kepler Architecture
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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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Semantic Scholar uses AI to extract papers important to this topic.
2015
2015
Spots on Am stars
L. Balona
,
G. Catanzaro
,
O. Abedigamba
,
V. Ripepi
,
B. Smalley
2015
Corpus ID: 96445195
We investigate the light variations of 15 Am stars using four years of high-precision photometry from the Kepler spacecraft and…
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Highly Cited
2015
Highly Cited
2015
CORRELATIONS BETWEEN COMPOSITIONS AND ORBITS ESTABLISHED BY THE GIANT IMPACT ERA OF PLANET FORMATION
R. Dawson
,
Eve J. Lee
,
E. Chiang
2015
Corpus ID: 118308826
The giant impact phase of terrestrial planet formation establishes connections between super-Earths’ orbital properties…
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Highly Cited
2014
Highly Cited
2014
CHARACTERIZING K2 PLANET DISCOVERIES: A SUPER-EARTH TRANSITING THE BRIGHT K DWARF HIP 116454
A. Vanderburg
,
B. Montet
,
+43 authors
W. Weiss
2014
Corpus ID: 3197176
We report the first planet discovery from the two-wheeled Kepler (K2) mission: HIP 116454 b. The host star HIP 116454 is a bright…
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Highly Cited
2014
Highly Cited
2014
MOST SUB-ARCSECOND COMPANIONS OF KEPLER EXOPLANET CANDIDATE HOST STARS ARE GRAVITATIONALLY BOUND
E. Horch
,
S. Howell
,
M. Everett
,
D. Ciardi
2014
Corpus ID: 25583970
Using the known detection limits for high-resolution imaging observations and the statistical properties of true binary and line…
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2014
2014
SEVEN-PERIOD ASTEROSEISMIC FIT OF THE KEPLER DBV
A. Bischoff-Kim
,
R. Østensen
,
J. Hermes
,
J. Provencal
2014
Corpus ID: 118482461
We present a new, better-constrained asteroseismic analysis of the helium-atmosphere (DB) white dwarf discovered in the field of…
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Review
2013
Review
2013
ASTEROSEISMIC CLASSIFICATION OF STELLAR POPULATIONS AMONG 13,000 RED GIANTS OBSERVED BY KEPLER
D. Stello
,
D. Huber
,
+7 authors
T. White
2013
Corpus ID: 119262509
Of the more than 150,000 targets followed by the Kepler Mission, about 10% were selected as red giants. Due to their high…
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2013
2013
KEPLER'S OPTICAL SECONDARY ECLIPSE OF HAT-P-7b AND PROBABLE DETECTION OF PLANET-INDUCED STELLAR GRAVITY DARKENING
B. Morris
,
A. Mandell
,
D. Deming
2013
Corpus ID: 119212074
We present observations spanning 355 orbital phases of HAT-P-7 observed by Kepler from 2009 May to 2011 March (Q1–9). We find a…
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2011
2011
AT LAST—A V777 HER PULSATOR IN THE KEPLER FIELD
R. Østensen
,
S. Bloemen
,
+5 authors
D. Koester
2011
Corpus ID: 55192759
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…
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2004
2004
The superposition image in the eye ofEphestia kühniella
P. Cleary
,
G. Deichsel
,
P. Kunze
Journal of Comparative Physiology
2004
Corpus ID: 41198359
SummarySuperposition images according to Exner (1891) are observed behind fresh eye-cups ofEphestia which were mounted with…
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Highly Cited
2003
Highly Cited
2003
Efficient Orbit Integration by Scaling for Kepler Energy Consistency
T. Fukushima
2003
Corpus ID: 56289338
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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