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20072026
most citedThe California-Kepler Survey. III. A Gap in the Radius Distribution of Small Planets

1.5k citations · 32.2k across the 408 of their papers we have counts for

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Showing 2013Show all

16 papers · 1 filter

astro-ph.EP2013★ 101 cited

What asteroseismology can do for exoplanets: Kepler-410A b is a Small Neptune around a bright star, in an eccentric orbit consistent with low obliquity

Vincent Van Eylen, Mikkel N. Lund, Victor Silva Aguirre +12

We confirm the Kepler planet candidate Kepler-410b (KOI-42b) as a Neptune sized exoplanet on a 17.8 day, eccentric orbit around the bright (Kp = 9.4) star Kepler-410A. This is the…

astro-ph.EP2013★ 64 cited

The TRENDS High-Contrast Imaging Survey. V. Discovery of an Old and Cold Benchmark T-dwarf Orbiting the Nearby G-star HD 19467

Justin R. Crepp, John Asher Johnson, Andrew W. Howard +5

The nearby Sun-like star HD 19467 shows a subtle radial velocity (RV) acceleration of -1.37+/-0.09 m/s/yr over an 16.9 year time baseline (an RV trend), hinting at the existence of…

astro-ph.EP2013★ 176 cited

A Rocky Composition for an Earth-sized Exoplanet

Andrew W. Howard, Roberto Sanchis-Ojeda, Geoffrey W. Marcy +7

Planets with sizes between that of Earth (with radius R) and Neptune (about 4 R) are now known to be common around Sun-like stars. Most such planets have been dis…

astro-ph.EP2013★ 318 cited

Stellar Spin-Orbit Misalignment in a Multiplanet System

Daniel Huber, Joshua A. Carter, Mauro Barbieri +32

Stars hosting hot Jupiters are often observed to have high obliquities, whereas stars with multiple co-planar planets have been seen to have low obliquities. This has been interpre…

astro-ph.EP2013★ 159 cited

Kepler-63b: A Giant Planet in a Polar Orbit around a Young Sun-like Star

Roberto Sanchis-Ojeda, Joshua N. Winn, Geoffrey W. Marcy +19

We present the discovery and characterization of a giant planet orbiting the young Sun-like star Kepler-63 (KOI-63, , K, $M_\star = 0.98\, M…

astro-ph.EP2013★ 129 cited

The same frequency of planets inside and outside open clusters of stars

Søren Meibom, Guillermo Torres, Francois Fressin +16

Most stars and their planets form in open clusters. Over 95 per cent of such clusters have stellar densities too low (less than a hundred stars per cubic parsec) to withstand inter…