activity
20122026
most citedSuperflares on Solar Type Stars Observed with Kepler I. Statistical Properties of Superflares

492 citations · 2.9k across the 71 of their papers we have counts for

collaborators

78 papers

astro-ph.SR2026

Frequent X-class Far UV Flares from a Young Solar Analog DS Tucanae A

Tristen Sextro, Kevin France, Vladimir Airapetian +4

The young solar analog DS Tuc A (~45 million years old, spectral type G6V) serves as an excellent proxy to the Sun during early stages of the Earth's evolution. The young Sun's enh…

astro-ph.SR2026

Systematic and Statistical Properties of Prominence Eruptions on the M-dwarf YZ CMi

Yuto Kajikiya, Kosuke Namekata, Yuta Notsu +4

M-dwarfs produce frequent flares, and their associated mass ejections are expected to significantly affect the habitability of close-in exoplanets. Recent spectroscopic observation…

astro-ph.SR2026

Broadband 12-26 GHz Radio Radiation Reveals Evidence for Micro-flares on AU Mic

Isaiah I. Tristan, Rachel A. Osten, Yuta Notsu +2

We present sequential 12-18 and 18-26 GHz radio-band (, ) VLA observations of the 22 Myr dM1e star AU Mic. We detect two flares and two marginal events over a total of 3 con…

astro-ph.SR2026

Magnetic Heating Across the Sun and Solar-like Stars: Universal Scaling Laws from Chromospheres to Coronae

Shin Toriumi, Kosuke Namekata, Yuta Notsu +2

Magnetic activity in cool stars governs the thermal structure and high-energy radiative output of their outer atmospheres, thereby influencing stellar evolution, stellar winds, and…

astro-ph.EP2026

ESCAPE: a small explorer mission to study the stellar drivers of exoplanet evolution

Allison Youngblood, Kevin France, Brian Fleming +37

The long-term stability of exoplanetary atmospheres depends critically on the extreme-ultraviolet (EUV) photon and high-energy particle fluxes from the host star, which are poorly…

astro-ph.SR2026

Stellar Forcing of (exo)Planetary Environments

Julián D. Alvarado-Gómez, Erika Palmerio, Manuel Güdel +13

The environments of exoplanets are fundamentally shaped by the magnetic activity of their host stars through radiative, plasma, and particle-driven processes. This article presents…