output
19932026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations

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128 papers · 1 filter

astro-ph.SR2025

Magnetic activity and differential rotation of HIP12653

Amina Boulkaboul, Lotfi Yelles Chaouche, Alessandro C. Lanzafame +1

We present a spectroscopic and photometric study of HIP12653 to investigate its magnetic cycle and differential rotation. Using HARPS archival spectra matched with MARCS-AMBER theo…

astro-ph.SR2025

CUbesat Solar Polarimeter (CUSP) Sensitivity Estimation and Performance Optimization using Geant4

Abhay Kumar, Giovanni Lombardi, Giovanni De Cesare +45

The CUbesat Solar Polarimeter (CUSP) aims to measure the linear polarization of solar flares in the 25-100 keV X-ray band using a Compton scattering polarimeter. CUSP will allow us…

astro-ph.SR2025★ 5 cited

Four ages of rotating stars in the rotation--activity relationship and gyrochronology

Huiqin Yang, Jifeng Liu, Roberto Soria +4

Gyrochronology and the rotation--activity relationship are standard techniques used to determine the evolution phase.The mismatch in the definition of the evolutionary phases has s…

astro-ph.SR2025★ 3 cited

The stellar population in the SARAO MeerKAT Galactic Plane Survey

Okwudili D. Egbo, David A. H. Buckley, Paul J. Groot +5

We report on optically selected stellar candidates of SARAO MeerKAT 1.3 GHz radio continuum survey sources of the Galactic plane. Stellar counterparts to radio sources are selected…

astro-ph.SR2024★ 2 cited

Gravity's role in taming the Tayler instability in red giant cores

Domenico G. Meduri, Rainer Arlt, Alfio Bonanno +1

The stability of toroidal magnetic fields in radiative stellar interiors is a key open problem in astrophysics. We investigate the Tayler instability of purely toroidal fields $B_ϕ…

astro-ph.SR2024★ 5 cited

Understanding the thermal and magnetic properties of a X-class flare in the low solar atmosphere

F. Ferrente, C. Quintero Noda, F. Zuccarello +1

We analyse the spatial distribution and vertical stratification of the physical parameters of the solar atmosphere when an X-class flare occurs. We made use of observations acquire…