activity
20142026
most citedProbing the physics of the solar atmosphere with the Multi-slit Solar Explorer (MUSE): I. Coronal Heating

81 citations · 481 across the 34 of their papers we have counts for

collaborators

35 papers

astro-ph.EP2026

The GAPS Programme at TNG. LXXX. Characterisation of the 400 Myr old multi-planet system K2-233

V. Fardella, S. Benatti, R. Spinelli +27

Understanding exoplanet physical properties is crucial for characterising their atmospheres and internal composition. Precise planetary masses are essential for constraining bulk d…

astro-ph.SR2026

MHD Modelling of magnetic reconnection heating and jets in the solar corona

P. Pagano, C. Argiroffi, F. Reale +3

Magnetic reconnection is seen as the lead mechanism to explain the persistent and bursty heating of the solar corona that keeps its thermal structure. Lately the observations and m…

astro-ph.EP2026★ 2 cited

True Masses using RV data with Hipparcos and Gaia Astrometry

G. Piccinini, A. Petralia, A. Sozzetti +3

Long-period companions are detected and characterized thanks to long-baseline radial velocity surveys. Combining Doppler time-series with astrometry, and in particular with proper…

astro-ph.SR2025

3D MHD simulations of coronal loops heated via magnetic braiding I. Continuous driving

Gabriele Cozzo, Paola Testa, Juan Martinez-Sykora +13

The nature and detailed properties of the heating of the million-degree solar corona are important issues that are still largely unresolved. Nanoflare heating might be dominant in…

astro-ph.SR2024

PAStar: a model for stellar surface from the Sun to active stars

Antonino Petralia, Jesús Maldonado, Giuseppina Micela

Context. The characterization of exoplanets requires a good description of the host star. Stellar activity acts as a source of noise which can alter planet radii as derived from th…

astro-ph.EP2024★ 3 cited

The GAPS programme at TNG -- LXIII. Photo-evaporating puzzle: Exploring the enigmatic nature of TOI-5398 b atmospheric signal

M. C. D'Arpa, G. Guilluy, G. Mantovan +26

Atmospheric characterization is key to understanding exoplanetary systems, offering insights into the planets current and past conditions. By analyzing key lines like H alpha and t…