activity
20082015
most citedHAT-P-14b: A 2.2 Jupiter-mass exoplanet transiting a bright F star

79 citations · 138 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2015★ 12 cited

HAT-P-55b: A Hot Jupiter Transiting a Sun-like Star

D. Juncher, L. A. Buchhave, J. D. Hartman +16

We report the discovery of a new transiting extrasolar planet, HAT-P-55b. The planet orbits a V = 13.207 +/- 0.039 sun-like star with a mass of 1.013 +/- 0.037 solar masses, a radi…

astro-ph.SR2015★ 8 cited

Precise mass and radius measurements for the components of the bright solar-type eclipsing binary star V1094 Tau

P. F. L. Maxted, R. J. Hutcheon, G. Torres +6

V1094 Tau is bright eclipsing binary star with an orbital period close to 9 days containing two stars similar to the Sun. Our aim is to test models of Sun-like stars using precise…

astro-ph.EP2010★ 79 cited

HAT-P-14b: A 2.2 Jupiter-mass exoplanet transiting a bright F star

G. Torres, G. A. Bakos, J. Hartman +16

We report the discovery of HAT-P-14b, a fairly massive transiting extrasolar planet orbiting the moderately bright star GSC 3086-00152 (V = 9.98), with a period of P = 4.627669 +/-…

astro-ph.SR2009★ 21 cited

Absolute properties of the highly eccentric eclipsing binary star LV Herculis

Guillermo Torres, Claud H. Sandberg Lacy, Antonio Claret

We report extensive spectroscopic and differential V-band photometric observations of the 18.4-day detached double-lined eclipsing binary LV Her (F9V), which has the highest eccent…

astro-ph2008

Absolute dimensions of the F-type eclipsing binary star VZ Cephei

Guillermo Torres, Claud H. Sandberg Lacy

We present new V-band differential photometry and radial-velocity measurements of the unevolved 1.18-day period F+G-type double-lined eclipsing binary VZ Cep. We determine accurate…

astro-ph2008★ 18 cited

Absolute properties of the spotted eclipsing binary star CV Bootis

Guillermo Torres, Luiz Paulo R. Vaz, Claud H. Sandberg Lacy

We present new V-band differential brightness measurements as well as new radial-velocity measurements of the detached, circular, 0.84-day period, double-lined eclipsing binary sys…