activity
20222025
most citedThe GAPS Programme at TNG XXXVIII. Five molecules in the atmosphere of the warm giant planet WASP-69b detected at high spectral resolution

50 citations · 215 across the 11 of their papers we have counts for

collaborators

5 papers

astro-ph.EP202511 cited

Characterizing WASP-43b's interior structure: unveiling tidal decay and apsidal motion

Lia Marta Bernabò, Szilárd Csizmadia, Alexis M. S. Smith +8

Context. Recent developments in exoplanetary research highlight the importance of Love numbers in understanding their internal dynamics, formation, migration history and their pote…

astro-ph.EP202215 cited

Characterization of exoplanetary atmospheres with SLOPpy

Daniela Sicilia, Luca Malavolta, Lorenzo Pino +4

Transmission spectroscopy is among the most fruitful techniques to infer the main opacity sources present in the upper atmosphere of a transiting planet and to constrain the compos…

astro-ph.EP202229 cited

Unifying High- and Low-resolution Observations to Constrain the Dayside Atmosphere of KELT-20b/MASCARA-2b

David Kasper, Jacob L. Bean, Michael R. Line +10

We present high-resolution dayside thermal emission observations of the exoplanet KELT-20b/MASCARA-2b using the MAROON-X spectrograph. Applying the cross-correlation method with bo…

astro-ph.EP202250 cited

The GAPS Programme at TNG XXXVIII. Five molecules in the atmosphere of the warm giant planet WASP-69b detected at high spectral resolution

G. Guilluy, P. Giacobbe, I. Carleo +32

The field of exo-atmospheric characterisation is progressing at an extraordinary pace. Atmospheric observations are now available for tens of exoplanets, mainly hot and warm inflat…

astro-ph.EP202239 cited

The GAPS Programme at TNG XXXIX -- Multiple molecular species in the atmosphere of the warm giant planet WASP-80 b unveiled at high resolution with GIANO-B

Ilaria Carleo, Paolo Giacobbe, Gloria Guilluy +28

Detections of molecules in the atmosphere of gas giant exoplanets allow us to investigate the physico-chemical properties of the atmospheres. Their inferred chemical composition is…