activity
19972022
most citedStrong Water Absorption in the Dayside Emission Spectrum of the Planet HD 189733b

300 citations · 736 across the 27 of their papers we have counts for

collaborators

27 papers

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.IM2019★ 46 cited

Precise Radial Velocities of Cool Low Mass Stars With iSHELL

Bryson Cale, Peter Plavchan, Danny LeBrun +11

The coolest dwarf stars are intrinsically faint at visible wavelengths and exhibit rotationally modulated stellar activity from spots and plages. It is advantageous to observe thes…

astro-ph.SR2019

Astro2020 Science White Paper: High Angular Resolution Astrophysics - Fundamental Stellar Parameters

Gerard van Belle, Ellyn Baines, Tabetha Boyajian +8

Direct determination of fundamental stellar parameters has many profound and wide-ranging impacts throughout astrophysics. These determinations are rooted in high angular resolutio…

astro-ph.SR2019★ 15 cited

Benchmarking Substellar Evolutionary Models Using New Age Estimates for HD 4747 B and HD 19467 B

Charlotte M. Wood, Tabetha Boyajian, Kaspar von Braun +5

Constraining substellar evolutionary models (SSEMs) is particularly difficult due to a degeneracy between the mass, age, and luminosity of a brown dwarf. In cases where a brown dwa…

astro-ph.SR2017★ 69 cited

Predicting Stellar Angular Diameters from , , , Photometry

Arthur D. Adams, Tabetha S. Boyajian, Kaspar von Braun

Determining the physical properties of microlensing events depends on having accurate angular sizes of the source star. Using long-baseline optical interferometry we are able to me…

astro-ph.EP2017★ 11 cited

Extrasolar Planets and Their Host Stars

Kaspar von Braun, Tabetha Boyajian

In order to understand the exoplanet, you need to understand its parent star. Astrophysical parameters of extrasolar planets are directly and indirectly dependent on the properties…