activity
20142020
most citedHigh-resolution confirmation of an extended helium atmosphere around WASP-107b

135 citations · 632 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.EP202039 cited

MOVES III. Simultaneous X-ray and ultraviolet observations unveiling the variable environment of the hot Jupiter HD 189733b

V. Bourrier, P. J. Wheatley, A. Lecavelier des Etangs +8

In this third paper of the MOVES (Multiwavelength Observations of an eVaporating Exoplanet and its Star) programme, we combine Hubble Space Telescope far-ultraviolet observations w…

astro-ph.EP201975 cited

Wind of Change: retrieving exoplanet atmospheric winds from high-resolution spectroscopy

J. V. Seidel, D. Ehrenreich, L. Pino +5

Context. The atmosphere of exoplanets has been studied extensively in recent years, using numerical models to retrieve chemical composition, dynamical circulation or temperature fr…

astro-ph.EP201946 cited

WASP-52b. The effect of starspot correction on atmospheric retrievals

Giovanni Bruno, Nikole K. Lewis, Munazza K. Alam +13

We perform atmospheric retrievals on the full optical to infrared () transmission spectrum of the inflated hot Jupiter WASP-52b by combining HST/STIS, WFC3 IR…

astro-ph.EP201947 cited

The SOPHIE search for northern extrasolar planets. XIV. A temperate ( K) super-earth around the nearby star Gliese 411

R. F. Díaz, X. Delfosse, M. J. Hobson +33

Periodic radial velocity variations in the nearby M-dwarf star Gl411 are reported, based on measurements with the SOPHIE spectrograph. Current data do not allow us to distinguish b…

astro-ph.SR20191 cited

EUV observations of cool dwarf stars

Allison Youngblood, Jeremy Drake, James Mason +15

The EUV (100-912 Å) is a spectral region notoriously difficult to observe due to attenuation by neutral hydrogen gas in the interstellar medium. Despite this, hundreds to thousands…

astro-ph.EP2019

EUV influences on exoplanet atmospheric stability and evolution

Allison Youngblood, Kevin France, Tommi Koskinen +15

The planetary effective surface temperature alone is insufficient to characterize exoplanet atmospheres and their stability or evolution. Considering the star-planet system as a wh…