activity
20162022
most citedSix transiting planets and a chain of Laplace resonances in TOI-178

195 citations · 1.5k across the 26 of their papers we have counts for

collaborators

37 papers

astro-ph.EP2022130 cited

A candidate short-period sub-Earth orbiting Proxima Centauri

J. P. Faria, A. Suárez Mascareño, P. Figueira +34

Proxima Centauri is the closest star to the Sun. This small, low-mass, mid M dwarf is known to host an Earth-mass exoplanet with an orbital period of 11.2 days within the habitable…

astro-ph.EP202210 cited

CaRM: Exploring the chromatic Rossiter-McLaughlin effect. The cases of HD 189733b and WASP-127b

E. Cristo, N. C. Santos, O. Demangeon +34

In this paper we introduce CaRM, a semi-automatic code for the retrieval of broadband transmission spectra of transiting planets through the chromatic Rossiter-McLaughlin method. W…

astro-ph.EP202166 cited

The Rossiter-McLaughlin effect Revolutions: An ultra-short period planet and a warm mini-Neptune on perpendicular orbits

V. Bourrier, C. Lovis, M. Cretignier +34

Comparisons of the alignment of exoplanets with a common host star can be used to distinguish among concurrent evolution scenarios. However, multi-planet systems usually host mini-…

astro-ph.EP202118 cited

HD22496b: the first ESPRESSO standalone planet discovery

J. Lillo-Box, J. P. Faria, A. Suárez Mascareño +32

The ESPRESSO spectrograph is a new powerful tool to detect and characterize extrasolar planets. Its design allows unprecedented radial velocity precision (down to a few tens of cm/…

astro-ph.EP2021107 cited

Warm terrestrial planet with half the mass of Venus transiting a nearby star

Olivier D. S. Demangeon, M. R. Zapatero Osorio, Y. Alibert +42

The advent of a new generation of radial velocity instruments has allowed us to break the one Earth-mass barrier. We report a new milestone in this context with the detection of th…

astro-ph.EP202112 cited

A super-Earth on a close-in orbit around the M1V star GJ 740. A HADES and CARMENES collaboration

B. Toledo-Padrón, A. Suárez Mascareño, J. I. González Hernández +23

M-dwarfs have proven to be ideal targets for planetary radial velocity (RV) searches due to their higher planet-star mass contrast. The HADES and CARMENES programs aim to carry out…