activity
20172021
most citedAn ultrahot gas-giant exoplanet with a stratosphere

271 citations · 849 across the 12 of their papers we have counts for

collaborators

23 papers

astro-ph.EP20222 cited

UV Absorption by Silicate Cloud Precursors in Ultra-hot Jupiter WASP-178b

Joshua D. Lothringer, David K. Sing, Zafar Rustamkulov +6

Aerosols have been found to be nearly ubiquitous in substellar atmospheres. The precise temperature at which these aerosols begin to form in exoplanets has yet to be observationall…

astro-ph.EP20222 cited

Mass loss by atmospheric escape from extremely close-in planets

Tommi Koskinen, Panayotis Lavvas, Chenliang Huang +3

We explore atmospheric escape from close-in exoplanets with the highest mass loss rates. First, we locate the transition from stellar X-ray and UV-driven escape to rapid Roche lobe…

astro-ph.EP202111 cited

Energy deposition in Saturn's equatorial upper atmosphere

J. M. Chadney, T. T. Koskinen, X. Hu +6

We construct Saturn equatorial neutral temperature and density profiles of H, H, He, and CH, between 10 and 1 bar using measurements from Cassini's Ion Neutral Mass…

astro-ph.EP2021

Pluto's atmosphere observations with ALMA: spatially-resolved maps of CO and HCN emission and first detection of HNC

E. Lellouch, B. Butler, R. Moreno +6

Following the detection of CO and HCN in Pluto's atmosphere, we report on new ALMA observations of Pluto with two main goals: (i) obtaining spatially-resolved measurements (~0.06''…

astro-ph.EP20214 cited

The near-UV transit of HD 189733b with the XMM-Newton Optical Monitor

George W. King, Lía Corrales, Peter J. Wheatley +6

We present analysis of XMM-Newton Optical Monitor observations in the near-ultraviolet of HD 189733, covering twenty primary transits of its hot Jupiter planet. The transit is clea…

astro-ph.EP2021

HST PanCET program: Non-detection of atmospheric escape in the warm Saturn-sized planet WASP-29 b

L. A. dos Santos, V. Bourrier, D. Ehrenreich +10

(Abridged) Short-period gas giant exoplanets are susceptible to intense atmospheric escape due to their large scale heights and strong high-energy irradiation. This process is thou…