activity
20142024
most citedA Precise Water Abundance Measurement for the Hot Jupiter WASP-43b

417 citations · 1.6k across the 18 of their papers we have counts for

collaborators

16 papers

astro-ph.EP2023

On the Effectiveness of the Planetary Infrared Excess (PIE) Technique to Retrieve the Parameters of Multiplanet Systems around M dwarfs: A Case Study on the TRAPPIST-1 System

L. C. Mayorga, J. Lustig-Yaeger, K. B. Stevenson

The planetary infrared excess (PIE) technique has the potential to efficiently detect and characterize the thermal spectra of both transiting and non-transiting exoplanets. However…

astro-ph.EP20231 cited

Detection of Carbon Monoxide in the Atmosphere of WASP-39b Applying Standard Cross-Correlation Techniques to JWST NIRSpec G395H Data

Emma Esparza-Borges, Mercedes López-Morales, Jéa I. Adams Redai +30

Carbon monoxide was recently reported in the atmosphere of the hot Jupiter WASP-39b using the NIRSpec PRISM transit observation of this planet, collected as part of the JWST Transi…

astro-ph.EP20232 cited

Mass Derivation of planets K2-21b and K2-21c from Transit Timing Variations

Maryame El Moutamid, Kevin B. Stevenson, Billy Quarles +5

While various indirect methods are used to detect exoplanets, one of the most effective and accurate methods is the transit method, which measures the brightness of a given star fo…

astro-ph.EP2023164 cited

A reflective, metal-rich atmosphere for GJ 1214b from its JWST phase curve

Eliza M. -R. Kempton, Michael Zhang, Jacob L. Bean +30

There are no planets intermediate in size between Earth and Neptune in our Solar System, yet these objects are found around a substantial fraction of other stars. Population statis…

astro-ph.EP202322 cited

Detection of carbon monoxide's 4.6 micron fundamental band structure in WASP-39b's atmosphere with JWST NIRSpec G395H

David Grant, Joshua D. Lothringer, Hannah R. Wakeford +28

Carbon monoxide (CO) is predicted to be the dominant carbon-bearing molecule in giant planet atmospheres, and, along with water, is important for discerning the oxygen and therefor…

astro-ph.IM2022

The UV-SCOPE Mission: Ultraviolet Spectroscopic Characterization Of Planets and their Environments

David R. Ardila, Evgenya Shkolnik, John Ziemer +22

UV-SCOPE is a mission concept to determine the causes of atmospheric mass loss in exoplanets, investigate the mechanisms driving aerosol formation in hot Jupiters, and study the in…