activity
20022026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations · 12.8k across the 96 of their papers we have counts for

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26 papers · 1 filter

astro-ph.SR2026

Gaia method paper: an algorithm to detect flare events in Gaia time-series

E. Distefano, A. C. Lanzafame, A. F. Lanza +14

The third Gaia data release (GDR3) includes the gdr3_rotmod catalogue of 474026 stars with variability that is attributed to magnetic activity analogous to that observed in the Sun…

astro-ph.SR2025

Selection and characterisation of the M-dwarf targets in the PLATO Input Catalogue

L. Prisinzano, M. Montalto, G. Piotto +33

The ESA's PLAnetary Transits and Oscillations of Stars (PLATO) mission aims to detect planets orbiting around dwarfs and subgiant stars with spectral type F5 or later, including M-…

astro-ph.SR2024

The curious case of 2MASS J15594729+4403595, an ultra-fast M2 dwarf with possible Rieger cycles

S. Messina, G. Catanzaro, A. F. Lanza +4

RACE-OC (Rotation and ACtivity Evolution in Open Clusters) is a project aimed at characterising the rotational and magnetic activity properties of the late-type members of open clu…

astro-ph.SR2024★ 6 cited

Atmospheric heating and magnetism driven by Ne distillation in isolated white dwarfs

A. F. Lanza, N. Z. Rui, J. Farihi +2

The origin of atmospheric heating in the cool, magnetic white dwarf GD 356 remains unsolved nearly 40 years after its discovery. This once idiosyncratic star with $T_{\rm eff}\appr…

astro-ph.SR2024

Measuring stellar surface rotation and activity with the PLATO mission -- I. Strategy and application to simulated light curves

S. N. Breton, A. F Lanza, S. Messina +20

The Planetary Transits and Oscillations of stars mission (PLATO) will allow us to measure surface rotation and monitor photometric activity of tens of thousands of main sequence so…

astro-ph.SR2023

The GAPS programme at TNG LII. Spot modeling of V1298 Tau using SpotCCF tool

C. Di Maio, A. Petralia, G. Micela +27

The intrinsic variability due to the magnetic activity of young active stars is one of the main challenges in detecting and characterising exoplanets. We present a method able to m…