The largest ground-based catalogue of M-dwarf flares
A.D. Lavrukhina, B. Demkov, K. Malanchev, M.V. Pruzhinskaya, E.E.O. Ishida

TL;DR
This paper presents the largest ground-based catalogue of M-dwarf flares, analyzing over a billion measurements to identify and characterize 1,229 flare events, revealing correlations with spectral subtype and Galactic height.
Contribution
It introduces a machine-learning pipeline for flare detection in large-scale survey data and provides a comprehensive catalogue with detailed flare properties and statistical analyses.
Findings
Flare energies range from 10^31 to 10^35 erg.
Flaring fraction decreases with Galactic height.
Flare frequency increases towards later M spectral types.
Abstract
We present the largest ground-based catalogue of M-dwarf flares to date, comprising 1,229 time-resolved events identified in Zwicky Transient Facility Data Release 17. Using high-cadence ZTF observations collected between April 2018 and September 2020, we analyzed over 93 million variable light curves containing 4.1 billion photometric measurements. Flare candidates were identified through a machine-learning pipeline trained on simulated light curves generated by injecting TESS-based flare templates into ZTF data and then refined through an extensive post-filtering stage combining an additional classifier, metadata checks, and human inspection. For 655 flares with reliable Gaia-based distances and well-sampled light curves, we derived bolometric energies ranging from 10^31 to 10^35 erg. A clear correlation is observed between flare frequency and spectral subtype, with a sharp increase…
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