activity
20122026
most citedESPRESSO@VLT -- On-sky performance and first results

537 citations · 11.3k across the 206 of their papers we have counts for

collaborators
Showing 2018Show all

16 papers · 1 filter

astro-ph.EP2018★ 206 cited

Hubble PanCET: An extended upper atmosphere of neutral hydrogen around the warm Neptune GJ 3470 b

V. Bourrier, A. Lecavelier des Etangs, D. Ehrenreich +16

GJ 3470b is a warm Neptune transiting an M-dwarf star at the edge of the evaporation desert. It offers the possibility of investigating how low-mass, close-in exoplanets evolve und…

astro-ph.EP2018★ 96 cited

Detection of Helium in the Atmosphere of the Exo-Neptune HAT-P-11b

Megan Mansfield, Jacob L. Bean, Antonija Oklopčić +11

The helium absorption triplet at a wavelength of 10,833 Å has been proposed as a way to probe the escaping atmospheres of exoplanets. Recently this feature was detected for the fir…

astro-ph.EP2018★ 243 cited

Spectrally resolved helium absorption from the extended atmosphere of a warm Neptune-mass exoplanet

R. Allart, V. Bourrier, C. Lovis +7

Stellar heating causes atmospheres of close-in exoplanets to expand and escape. These extended atmospheres are difficult to observe because their main spectral signature - neutral…

astro-ph.EP2018★ 12 cited

Observability of hydrogen-rich exospheres in Earth-like exoplanets

Leonardo A. dos Santos, Vincent Bourrier, David Ehrenreich +1

(Abridged) The existence of an extended neutral hydrogen exosphere around small planets can be used as an evidence for the presence of water in their lower atmosphere but, to date,…

astro-ph.SR2018★ 12 cited

Detection of Nitrogen gas in the Pictoris circumstellar disk

P. A. Wilson, R. Kerr, A. Lecavelier des Etangs +4

The debris disk surrounding Pictoris has a gas composition rich in carbon and oxygen, relative to solar abundances. Two possible scenarios have been proposed to explain this en…

astro-ph.EP2018★ 100 cited

Disentangling the planet from the star in late type M dwarfs: A case study of TRAPPIST-1g

Hannah R. Wakeford, Nikole K. Lewis, Julia Fowler +10

The atmospheres of late M stars represent a significant challenge in the characterization of any transiting exoplanets due to the presence of strong molecular features in the stell…