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20142024
most citedOxygen depletion in giant planets with different formation histories

24 citations · 65 across the 6 of their papers we have counts for

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astro-ph.EP20248 cited

The GAPS programme at TNG LXIV: An inner eccentric sub-Neptune and an outer sub-Neptune-mass candidate around BD+00 444 (TOI-2443)

L. Naponiello, A. S. Bonomo, L. Mancini +25

We examined in depth the star BD+00 444 (GJ 105.5, TOI-2443; V = 9.5 mag; d = 23.9 pc), with the aim of characterizing and confirming the planetary nature of its small companion, t…

astro-ph.EP20249 cited

TOI-837 b: characterisation, formation and evolutionary history of an infant warm Saturn-mass planet

M. Damasso, D. Polychroni, D. Locci +15

We aim to determine the fundamental properties of the 35 Myr old star TOI-837 and its close-in Saturn-sized planet, and to investigate the system's formation and evolutionary…

astro-ph.EP2024

Orbital obliquity of the young planet TOI-5398 b and the evolutionary history of the system

G. Mantovan, L. Malavolta, D. Locci +19

Multi-planet systems exhibit remarkable architectural diversity. However, short-period giant planets are typically isolated. Compact systems like TOI-5398, with an outer close-orbi…

astro-ph.EP20232 cited

The GAPS programme at TNG XLIX. TOI-5398, the youngest compact multi-planet system composed of an inner sub-Neptune and an outer warm Saturn

G. Mantovan, L. Malavolta, S. Desidera +68

Short-period giant planets are frequently found to be solitary compared to other classes of exoplanets. Small inner companions to giant planets with 15 days are known…

astro-ph.EP202318 cited

The GAPS program at TNG XLVII: The unusual formation history of V1298 Tau

D. Turrini, F. Marzari, D. Polychroni +33

Observational data from space and ground-based campaigns reveal that the 10-30 Ma old V1298 Tau star hosts a compact and massive system of four planets. Mass estimates for the two…

astro-ph.EP202324 cited

Oxygen depletion in giant planets with different formation histories

S. Fonte, D. Turrini, E. Pacetti +5

The atmospheric C/O ratio of exoplanets is widely used to constrain their formation. To guarantee that the C/O ratio provides robust information, we need to accurately quantify the…