most citedA precise architecture characterization of the Men planetary system

62 citations · 118 across the 5 of their papers we have counts for

collaborators

7 papers

astro-ph.EP202062 cited

A precise architecture characterization of the Men planetary system

M. Damasso, A. Sozzetti, C. Lovis +97

The bright star Men was chosen as the first target for a radial velocity follow-up to test the performance of ESPRESSO, the new high-resolution spectrograph at the ESO's Very-L…

astro-ph.EP202036 cited

Characterization of the K2-38 planetary system. Unraveling one of the densest planets known to date

B. Toledo-Padrón, C. Lovis, A. Suárez Mascareño +90

We characterized the transiting planetary system orbiting the G2V star K2-38 using the new-generation echelle spectrograph ESPRESSO. We carried out a photometric analysis of the av…

astro-ph.EP2020

Nightside condensation of iron in an ultra-hot giant exoplanet

David Ehrenreich, Christophe Lovis, Romain Allart +94

Ultra-hot giant exoplanets receive thousands of times Earth's insolation. Their high-temperature atmospheres (>2,000 K) are ideal laboratories for studying extreme planetary climat…

astro-ph.IM201915 cited

The impact of atmospheric dispersion in the performance of high-resolution spectrographs

Bachar Wehbe, Alexandre Cabral, Jorge Martins +3

Differential atmospheric dispersion is a wavelength-dependent effect introduced by the atmosphere. It is one of the instrumental errors that can affect the position of the target a…

astro-ph.IM20193 cited

The development of an optical design tool for atmospheric dispersion correction

Bachar Wehbe, Alexandre Cabral, Gerardo Avila

In ground based astronomical observations, atmospheric dispersion shifts the image of the object at different wavelengths due to the wavelength-dependent index of refraction of the…

astro-ph.IM20192 cited

Atmospheric dispersion correction: model requirements and impact on radial velocity measurements

Bachar Wehbe, Alexandre Cabral, Pedro Figueira +1

Observations with ground-based telescopes are affected by differential atmospheric dispersion when seen at a zenith angle different from zero, a consequence of the wavelength-depen…