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

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

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Showing 2024Show all

13 papers · 1 filter

astro-ph.EP2024★ 11 cited

ESPRESSO reveals blueshifted neutral iron emission lines on the dayside of WASP-76 b

A. R. Costa Silva, O. D. S. Demangeon, N. C. Santos +34

Ultra hot Jupiters (gas giants, Teq>2000 K) are intriguing exoplanets due to their extreme atmospheres. Their torrid daysides can be characterised using ground-based high-resolutio…

astro-ph.EP2024★ 49 cited

Mapping the exo-Neptunian landscape. A ridge between the desert and savanna

A. Castro-González, V. Bourrier, J. Lillo-Box +4

Atmospheric and dynamical processes are thought to play a major role in shaping the distribution of close-in exoplanets. A striking feature of such distribution is the Neptunian de…

astro-ph.EP2024★ 33 cited

TOI-5005 b: A super-Neptune in the savanna near the ridge

A. Castro-González, J. Lillo-Box, D. J. Armstrong +38

The Neptunian desert and savanna have recently been found to be separated by a ridge, an overdensity of planets in the period range of 3-5 days. These features are thought…

astro-ph.EP2024

The ANTARESS workflow I. Optimal extraction of spatially resolved stellar spectra with high-resolution transit spectroscopy

V. Bourrier, J. -B. Delisle, C. Lovis +17

High-resolution spectrographs open a detailed window onto the atmospheres of stars and planets. As the number of systems observed with different instruments grows, it is crucial to…

astro-ph.EP2024★ 38 cited

JWST reveals a rapid and strong day side variability of 55 Cancri e

J. A. Patel, A. Brandeker, D. Kitzmann +16

The nature of the close-in rocky planet 55 Cnc e is puzzling despite having been observed extensively. Its optical and infrared occultation depths show temporal variability, in add…

astro-ph.EP2024★ 22 cited

Resonant sub-Neptunes are puffier

Adrien Leleu, Jean-Baptiste Delisle, Remo Burn +12

A systematic, population-level discrepancy exists between the densities of exoplanets whose masses have been measured with transit timing variations (TTVs) versus those measured wi…