activity
20242026
most citedJWST Thermal Emission of the Terrestrial Exoplanet GJ 1132b

50 citations · 109 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2026★ 3 cited

Evidence for an Atmosphere on the Ultra-Short Period super-Earth HD 3167 b

Brandon Park Coy, Qiao Xue, Megan Weiner Mansfield +14

'Lava worlds'-Earth-sized planets hot enough (Teq >~ 1100 K) to melt their dayside silicate surfaces-have emerged as promising candidates for atmospheric detection and characteriza…

astro-ph.EP2025★ 23 cited

Hot Rocks Survey II: The thermal emission of TOI-1468 b reveals a hot bare rock

E. A. Meier Valdés, B. -O. Demory, H. Diamond-Lowe +17

Terrestrial exoplanets orbiting nearby small, cool stars known as M dwarfs are well suited for atmospheric characterisation. Given the strong XUV irradiation from M dwarf host star…

astro-ph.EP2024★ 32 cited

Hot Rocks Survey I : A possible shallow eclipse for LHS 1478 b

Prune C. August, Lars A. Buchhave, Hannah Diamond-Lowe +18

M dwarf systems offer an opportunity to study terrestrial exoplanetary atmospheres due to their small size and cool temperatures. However, the extreme conditions imposed by these h…

astro-ph.EP2024★ 50 cited

JWST Thermal Emission of the Terrestrial Exoplanet GJ 1132b

Qiao Xue, Jacob L. Bean, Michael Zhang +9

We present thermal emission measurements of GJ 1132b spanning 5--12 um obtained with the Mid-Infrared Instrument Low-Resolution Spectrometer (MIRI/LRS) on the James Webb Space Tele…

astro-ph.EP2024★ 1 cited

No Thick Atmosphere on the Terrestrial Exoplanet Gl 486b

Megan Weiner Mansfield, Qiao Xue, Michael Zhang +8

A primary science goal for JWST is to detect and characterize the atmospheres of terrestrial planets orbiting M dwarfs (M-Earths). The existence of atmospheres on M-Earths is highl…

astro-ph.EP2024

New insights into the internal structure of GJ 1214 b informed by JWST

Matthew C. Nixon, Anjali A. A. Piette, Eliza M. -R. Kempton +7

Recent JWST observations of the sub-Neptune GJ 1214 b suggest that it hosts a high-metallicity (>100x solar), hazy atmosphere. Emission spectra of the planet show molecular absorpt…