activity
20062023
most citedStellar Diameters and Temperatures II. Main Sequence K & M Stars

593 citations · 4.9k across the 82 of their papers we have counts for

collaborators

82 papers

astro-ph.SR2023★ 5 cited

Precise Age for the Binary Star System 12 Com in the Coma Berenices Cluster

Rex Lam, Eric L. Sandquist, Gail H. Schaefer +11

We present measurements of the interferometrically-resolved binary star system 12 Com and the single giant star 31 Com in the cluster Coma Berenices. 12 Com is a double-lined spect…

astro-ph.SR2022★ 9 cited

The Orbits and Dynamical Masses of the Castor System

Guillermo Torres, Gail H. Schaefer, John D. Monnier +12

Castor is a system of six stars in which the two brighter objects, Castor A and B, revolve around each other every 450 yr and are both short-period spectroscopic binaries. Th…

astro-ph.SR2022★ 6 cited

Visual Orbits of Spectroscopic Binaries with the CHARA Array. IV. HD 61859, HD 89822, HD 109510, and HD 191692

Kathryn V. Lester, Gail H. Schaefer, Francis C. Fekel +18

We present the visual orbits of four spectroscopic binary stars, HD 61859, HD 89822, HD 109510, and HD 191692, using long baseline interferometry with the CHARA Array. We also obta…

astro-ph.GA2022★ 15 cited

The dust sublimation region of the Type 1 AGN NGC4151 at a hundred micro-arcsecond scale as resolved by the CHARA Array interferometer

Makoto Kishimoto, Matt Anderson, Theo ten Brummelaar +10

The nuclear region of Type 1 AGNs has only been partially resolved so far in the near-infrared (IR) where we expect to see the dust sublimation region and the nucleus directly with…

astro-ph.EP2022★ 47 cited

A detailed analysis of the Gl 486 planetary system

J. A. Caballero, E. Gonzalez-Alvarez, M. Brady +64

The Gl 486 system consists of a very nearby, relatively bright, weakly active M3.5 V star at just 8 pc with a warm transiting rocky planet of about 1.3 R_Terra and 3.0 M_Terra that…

astro-ph.SR2022★ 11 cited

The Interferometric Binary Epsilon Cancri in Praesepe: Precise Masses and Age

Leslie M. Morales, Eric L. Sandquist, Gail H. Schaefer +16

We observe the brightest member of the Praesepe cluster, Epsilon Cancri, to precisely measure the characteristics of the stars in this binary system, en route to a new measurement…