activity
19962026
most citedSix transiting planets and a chain of Laplace resonances in TOI-178

195 citations · 3k across the 74 of their papers we have counts for

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Showing 2020Show all

24 papers · 1 filter

astro-ph.IM2020

LOCNES: a solar telescope to study stellar activity in the near infrared

Claudi R., Ghedina A., Pace E. +27

LOCNES (LOw-Cost NIR Extended Solar telescope) is a solar telescope installed at the TNG (Telescopio Nazionale Galileo). It feeds the light of the Sun into the NIR spectrograph GIA…

astro-ph.GA2020

Gaia Early Data Release 3: Acceleration of the solar system from Gaia astrometry

Gaia Collaboration, S. A. Klioner, F. Mignard +414

Context. Gaia Early Data Release 3 (Gaia EDR3) provides accurate astrometry for about 1.6 million compact (QSO-like) extragalactic sources, 1.2 million of which have the best-quali…

astro-ph.EP202039 cited

The GAPS Programme at TNG XXVIII -- A pair of hot-Neptunes orbiting the young star TOI-942

Ilaria Carleo, Silvano Desidera, Domenico Nardiello +48

Both young stars and multi-planet systems are primary objects that allow us to study, understand and constrain planetary formation and evolution theories. We validate the physical…

astro-ph.EP2020108 cited

ESPRESSO high resolution transmission spectroscopy of WASP-76b

H. M. Tabernero, M. R. Zapatero Osorio, R. Allart +87

Aims. We report on ESPRESSO high-resolution transmission spectroscopic observations of two primary transits of the highly-irradiated, ultra-hot Jupiter-size planet WASP-76b. We inv…

astro-ph.EP202027 cited

Broadband transmission spectroscopy of HD209458b with ESPRESSO: Evidence for Na, TiO, or both

N. C. Santos, E. Cristo, O. Demangeon +42

The detection and characterization of exoplanet atmospheres is currently one of the main drivers pushing the development of new observing facilities. In this context, high-resoluti…

astro-ph.SR202076 cited

HADES RV Programme with HARPS-N at TNG XII. The abundance signature of M dwarf stars with planets

J. Maldonado, G. Micela, M. Baratella +27

Most of our current knowledge on planet formation is still based on the analysis of main-sequence, solar-type stars. Conversely, detailed chemical studies of large samples of M-dwa…