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most citedGEMS JWST: Transmission spectroscopy of TOI-5205b reveals significant stellar contamination and a metal-poor atmosphere

6 citations · 14 across the 15 of their papers we have counts for

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astro-ph.EP2025

A carbon-rich atmosphere on a windy pulsar planet

Michael Zhang, Maya Beleznay, Timothy D. Brandt +17

A handful of enigmatic Jupiter-mass objects have been discovered orbiting pulsars. One such object, PSR\,J2322-2650b, uniquely resembles a hot Jupiter exoplanet due to its minimum…

astro-ph.EP2025

The radiative effects of photochemical hazes on the atmospheric circulation and phase curves of sub-Neptunes

Maria E. Steinrueck, Vivien Parmentier, Laura Kreidberg +13

Measuring the atmospheric composition of hazy sub-Neptunes like GJ~1214b through transmission spectroscopy is difficult because of the degeneracy between mean molecular weight and…

astro-ph.EP2025★ 6 cited

GEMS JWST: Transmission spectroscopy of TOI-5205b reveals significant stellar contamination and a metal-poor atmosphere

Caleb I. Cañas, Jacob Lustig-Yaeger, Shang-Min Tsai +21

Recent discoveries of transiting giant exoplanets () around M dwarfs (GEMS) present an opportunity to investigate their atmospheric compositions and…

astro-ph.EP2025

Statistical trends in JWST transiting exoplanet atmospheres

Guangwei Fu, Kevin B. Stevenson, David K. Sing +13

Our brains are hardwired for pattern recognition as correlations are useful for predicting and understanding nature. As more exoplanet atmospheres are being characterized with JWST…

astro-ph.EP2025★ 1 cited

TOI-421 b: A Hot Sub-Neptune with a Haze-Free, Low Mean Molecular Weight Atmosphere

Brian Davenport, Eliza M. -R. Kempton, Matthew C. Nixon +8

Common features of sub-Neptunes atmospheres observed to date include signatures of aerosols at moderate equilibrium temperatures (~500-800 K), and a prevalence of high mean molecul…