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20212026
most citedA Clear View of a Cloudy Brown Dwarf Companion from High-Resolution Spectroscopy

73 citations · 194 across the 9 of their papers we have counts for

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6 papers · 1 filter

astro-ph.EP2024★ 1 cited

The Compositions of Rocky Planets in Close-in Orbits Tend to be Earth-Like

Casey L. Brinkman, Lauren M. Weiss, Daniel Huber +54

Hundreds of exoplanets between 1-1.8 times the size of the Earth have been discovered on close in orbits. However, these planets show such a diversity in densities that some appear…

astro-ph.EP2022★ 14 cited

A Reanalysis of the Composition of K2-106b: an Ultra-short Period Super-Mercury Candidate

Romy Rodríguez Martínez, B. Scott Gaudi, Joseph G. Schulze +9

We present a reanalysis of the K2-106 transiting planetary system, with a focus on the composition of K2-106b, an ultra-short period, super-Mercury candidate. We globally model exi…

astro-ph.EP2022★ 73 cited

A Clear View of a Cloudy Brown Dwarf Companion from High-Resolution Spectroscopy

Jerry W. Xuan, Jason Wang, Jean-Baptiste Ruffio +37

Direct imaging studies have mainly used low-resolution spectroscopy () to study the atmospheres of giant exoplanets and brown dwarf companions, but the presence of clo…

astro-ph.EP2022★ 43 cited

Retrieving the C and O Abundances of HR 7672~AB: a Solar-Type Primary Star with a Benchmark Brown Dwarf

Ji Wang, Jared R. Kolecki, Jean-Baptiste Ruffio +30

A benchmark brown dwarf (BD) is a BD whose properties (e.g., mass and chemical composition) are precisely and independently measured. Benchmark BDs are valuable in testing theoreti…

astro-ph.EP2021★ 27 cited

Measuring Elemental Abundances of JWST Target Stars for Exoplanet Characterization I. FGK Stars

Jared R. Kolecki, Ji Wang

With the launch of the JWST, we will obtain more precise data for exoplanets than ever before. However, this data can only inform and revolutionize our understanding of exoplanets…

astro-ph.EP2021★ 6 cited

Searching For Transiting Planets Around Halo Stars. I. Sample Selection and Validation

Jared R. Kolecki, Ji Wang, Jennifer A. Johnson +3

By measuring the elemental abundances of a star, we can gain insight into the composition of its initial gas cloud -- the formation site of the star and its planets. Planet formati…