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19982023
most citedA Survey of Stellar Families: Multiplicity of Solar-Type Stars

1.9k citations · 57.7k across the 610 of their papers we have counts for

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Showing 2012Show all

18 papers · 1 filter

astro-ph.EP2012★ 20 cited

HAT-P-42b and HAT-P-43b. Two Inflated Transiting Hot Jupiters from the HATNet Survey

I. Boisse, J. Hartman, G. Bakos +20

First identified from the HATNet wide-field photometric survey, these candidate transiting planets were then followed-up with a variety of photometric observations. Determining the…

astro-ph.SR2012

Spectroscopic and Photometric Observations of Kepler Asteroseismic Targets

J. Molenda-Zakowicz, M. Jerzykiewicz, G. Kopacki +10

We summarize our ground-based program of spectroscopic and photometric observations of the asteroseismic targets of the Kepler space telescope. We have already determined atmospher…

astro-ph.EP2012★ 74 cited

KELT-3b: A Hot Jupiter Transiting a V=9.8 Late-F Star

Joshua Pepper, Robert J. Siverd, Thomas G. Beatty +31

We report the discovery of KELT-3b, a moderately inflated transiting hot Jupiter with a mass of 1.477 (-0.067, +0.066) M_J, and radius of 1.345 +/- 0.072 R_J, with an orbital perio…

astro-ph.EP2012★ 136 cited

HAT-P-39b--HAT-P-41b: Three Highly Inflated Transiting Hot Jupiters

J. D. Hartman, G. Á. Bakos, B. Béky +26

We report the discovery of three new transiting extrasolar planets orbiting moderately bright (V=11.1 to 12.4) F stars. The planets have periods of P = 2.6940 d to 4.4572 d, masses…

astro-ph.EP2012★ 147 cited

Two 'b's in the Beehive: The Discovery of the First Hot Jupiters in an Open Cluster

S. N. Quinn, R. J. White, D. W. Latham +12

We present the discovery of two giant planets orbiting stars in Praesepe (also known as the Beehive Cluster). These are the first known hot Jupiters in an open cluster and the only…

astro-ph.EP2012★ 391 cited

Kepler-36: A Pair of Planets with Neighboring Orbits and Dissimilar Densities

Joshua A. Carter, Eric Agol, William J. Chaplin +43

In the Solar system the planets' compositions vary with orbital distance, with rocky planets in close orbits and lower-density gas giants in wider orbits. The detection of close-in…