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20212026
most citedA candidate short-period sub-Earth orbiting Proxima Centauri

130 citations · 501 across the 17 of their papers we have counts for

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10 papers · 1 filter

astro-ph.EP2023

A compact multi-planet system transiting HIP 29442 (TOI-469) discovered by TESS and ESPRESSO. Radial velocities lead to the detection of transits with low signal-to-noise ratio

M. Damasso, J. Rodrigues, A. Castro-González +52

We followed-up with ESPRESSO the K0V star HIP 29442 (TOI-469), already known to host a validated sub-Neptune companion TOI-469.01. We aim to verify the planetary nature of TOI-469.…

astro-ph.EP2023★ 41 cited

Detection of a high-velocity sodium feature on the ultra-hot Jupiter WASP-121 b

J. V. Seidel, F. Borsa, L. Pino +19

Ultra-hot Jupiters, with their high equilibrium temperatures and resolved spectral lines, have emerged as a perfect testbed for new analysis techniques in the study of exoplanet at…

astro-ph.EP2022★ 25 cited

Planetary system around LTT 1445A unveiled by ESPRESSO: Multiple planets in a triple M-dwarf system

B. Lavie, F. Bouchy, C. Lovis +32

We present radial velocity follow-up obtained with ESPRESSO of the M-type star LTT 1445A (TOI-455), for which a transiting planet b with an orbital period of~5.4 days was detected…

astro-ph.EP2022★ 55 cited

Detection of barium in the atmospheres of the ultra-hot gas giants WASP-76b and WASP-121b

T. Azevedo Silva, O. D. S. Demangeon, N. C. Santos +33

High-resolution spectroscopy studies of ultra-hot Jupiters have been key in our understanding of exoplanet atmospheres. Observing into the atmospheres of these giant planets allows…

astro-ph.EP2022★ 38 cited

Automatic model-based telluric correction for the ESPRESSO data reduction software. Model description and application to radial velocity computation

R. Allart, C. Lovis, J. Faria +21

Ground-based high-resolution spectrographs are key instruments for several astrophysical domains. Unfortunately, the observed spectra are contaminated by the Earth's atmosphere. Wh…

astro-ph.EP2022★ 35 cited

A novel framework for semi-Bayesian radial velocities through template matching

A. M. Silva, J. P. Faria, N. C. Santos +28

The detection and characterization of an increasing variety of exoplanets has been in part possible thanks to the continuous development of high-resolution, stable spectrographs, a…

astro-ph.EP2022★ 41 cited

The polar orbit of the warm Neptune GJ436b seen with VLT/ESPRESSO

V. Bourrier, M. R. Zapatero Osorio, R. Allart +24

GJ436b might be the prototype of warm Neptunes that have undergone late migration induced by an outer companion. Precise determination of the orbital architecture of such systems i…

astro-ph.EP2022★ 130 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.EP2022★ 10 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.EP2021★ 4 cited

Retrieving the transmission spectrum of HD 209458b using CHOCOLATE: A new chromatic Doppler tomography technique

E. Esparza-Borges, M. Oshagh, N. Casasayas-Barris +29

Multiband photometric transit observations or low-resolution spectroscopy (spectro-photometry) are normally used to retrieve the broadband transmission spectra of transiting exopla…