activity
19992026
most citedKepler-16: A Transiting Circumbinary Planet

750 citations · 7.7k across the 76 of their papers we have counts for

collaborators

76 papers

astro-ph.SR2026

Long-term Spectroscopic Survey of the Hyades Cluster: The Binary Population

Guillermo Torres, Robert P. Stefanik, David W. Latham

We report the results of a radial velocity monitoring program in the Hyades region, carried out at the Center for Astrophysics over a period of more than 45 yr. Nearly 12,000 spect…

astro-ph.SR2024

Orbits and Dynamical Masses for Six Binary Systems in the Hyades Cluster

Guillermo Torres, Gail H. Schaefer, Robert P. Stefanik +8

We report long baseline interferometric observations with the CHARA Array that resolve six previously known double-lined spectroscopic binary systems in the Hyades cluster, with or…

astro-ph.SR2023

Orbits and Dynamical Masses for the Active Hyades Multiple System HD 284163

Guillermo Torres, Gail H. Schaefer, Robert P. Stefanik +16

We report near-infrared long-baseline interferometric observations of the Hyades multiple system HD 284163, made with the CHARA array, as well as almost 43 yr of high-resolution sp…

astro-ph.SR2023

Dynamical Masses for the Hyades Binary System vB 120

Guillermo Torres, Robert P. Stefanik, David W. Latham

We report spectroscopic observations of vB 120 (HD 30712), a 5.7 yr astrometric-spectroscopic binary system in the Hyades cluster. We combine our radial velocities with others from…

astro-ph.SR2021★ 3 cited

Dissecting the Quadruple Binary Hyad vA 351 -- Masses for three M Dwarfs and a White Dwarf

G. Fritz Benedict, Otto G. Franz, Elliott P. Horch +8

We extend results first announced by Franz et al. (1998), that identified vA 351 = H346 in the Hyades as a multiple star system containing a white dwarf. With Hubble Space Telescop…

astro-ph.SR2019★ 18 cited

Dynamical masses for the triple system HD 28363 in the Hyades cluster

Guillermo Torres, Robert P. Stefanik, David W. Latham

The star HD 28363 in the Hyades cluster has been known for over a century as a visual binary with a period of 40 yr. The secondary is, in turn, a single-lined spectroscopic binary…