activity
20012016
most citedStellar Companions to Stars with Planets

360 citations · 1.7k across the 27 of their papers we have counts for

collaborators

27 papers

astro-ph.SR2016★ 40 cited

The Age of the Directly-Imaged Planet Host Star Andromedae Determined From Interferometric Observations

Jeremy Jones, R. J. White, S. Quinn +4

Andromedae, an early type star that hosts a directly imaged low mass companion, is expected to be oblate due to its rapid rotational velocity ( = 162 $\mathrm{km…

astro-ph.EP2013★ 124 cited

HD 285507b: An Eccentric Hot Jupiter in the Hyades Open Cluster

S. N. Quinn, R. J. White, D. W. Latham +10

We report the discovery of the first hot Jupiter in the Hyades open cluster. HD 285507b orbits a V=10.47 K4.5V dwarf (; ) in a slightly ec…

astro-ph.IM2013★ 13 cited

A Compact High Energy Camera for the Cherenkov Telescope Array

M. K. Daniel, R. J. White, D. Berge +23

The Compact High Energy Camera (CHEC) is a camera-development project involving UK, US, Japanese and Dutch institutes for the dual-mirror Small-Sized Telescopes (SST-2M) of the Che…

astro-ph.HE2012★ 26 cited

A Stacked Analysis of Brightest Cluster Galaxies Observed with the Fermi Large Area Telescope

K. L. Dutson, R. J. White, A. C. Edge +2

We present the results of a search for high-energy gamma-ray emission from a large sample of galaxy clusters sharing the properties of three existing Fermi-LAT detections (in Perse…

astro-ph.EP2011★ 1 cited

The 55 Cancri System: Fundamental Stellar Parameters, Habitable Zone Planet, and Super-Earth Diameter

K. von Braun, T. S. Boyajian, T. A. ten Brummelaar +13

The bright star 55 Cancri is known to host five planets, including a transiting super-Earth. We use the CHARA Array to directly determine the following of 55 Cnc's stellar astrophy…

astro-ph.HE2009★ 44 cited

Multiwavelength Observations of LS I +61 303 with VERITAS, Swift and RXTE

VERITAS Collaboration, V. A. Acciari, E. Aliu +83

We present results from a long-term monitoring campaign on the TeV binary LSI +61 303 with VERITAS at energies above 500 GeV, and in the 2-10 keV hard X-ray bands with RXTE and Swi…