activity
20172025
most citedA solar C/O and sub-solar metallicity in a hot Jupiter atmosphere

186 citations · 292 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2025★ 2 cited

A Stellar Magnesium to Silicon ratio in the atmosphere of an exoplanet

Jorge A. Sanchez, Peter C. B. Smith, Krishna Kanumalla +17

The elemental compositions of exoplanets encode information about their formation environments and internal structures. While volatile ratios such as carbon-to-oxygen (C/O) are use…

astro-ph.SR2025★ 2 cited

A 1.48-2.48 m R=28000 spectroscopic atlas of the L7.5 and T0.5 components of the nearest pair of brown dwarfs: Luhman 16AB

Hiroyuki Tako Ishikawa, Stanimir Metchev, Megan E. Tannock +6

We present a high signal-to-noise (SNR 450), high-dispersion () H- and K-band spectroscopic atlas of the L7.5 and T0.5 components of the Luhman 1…

astro-ph.EP2024★ 34 cited

A giant planet transiting a 3-Myr protostar with a misaligned disk

Madyson G. Barber, Andrew W. Mann, Andrew Vanderburg +35

Astronomers have found more than a dozen planets transiting 10-40 million year old stars, but even younger transiting planets have remained elusive. A possible reason for the lack…

astro-ph.EP2024★ 24 cited

A sub-solar metallicity on the ultra-short period planet HIP 65Ab

Luc Bazinet, Stefan Pelletier, Björn Benneke +2

Studying and understanding the physical and chemical processes that govern hot Jupiters gives us insights on the formation of these giant planets. Having a constraint on the molecu…

astro-ph.EP2021★ 186 cited

A solar C/O and sub-solar metallicity in a hot Jupiter atmosphere

Michael R. Line, Matteo Brogi, Jacob L. Bean +13

Measurements of the atmospheric carbon (C) and oxygen (O) relative to hydrogen (H) in hot Jupiters (relative to their host stars) provide insight into their formation location and…

astro-ph.SR2017★ 44 cited

EPIC 220204960: A Quadruple Star System Containing Two Strongly Interacting Eclipsing Binaries

S. Rappaport, A. Vanderburg, T. Borkovits +15

We present a strongly interacting quadruple system associated with the K2 target EPIC 220204960. The K2 target itself is a Kp = 12.7 magnitude star at Teff ~ 6100 K which we design…