The Deeper, Wider, Faster programme: exploring stellar flare activity with deep, fast cadenced DECam imaging via machine learning. Issue 2 (28th June 2021)

• Record Type: Journal Article
• Authors: Webb, S; Flynn, C; Cooke, J; Zhang, J; Mahabal, A; Abbott, T M C; Allen, R; Andreoni, I; Bird, S A; Goode, S; Lochner, M; Pritchard, T
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 506:Issue 2(2021)
• Page Start: 2089
• Page End: 2103
• Publication Date: 2021-06-28
• Subjects: methods: data analysis -- parallaxes -- stars: flare -- stars: low-mass; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stab1798
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: We present our 500 pc distance-limited study of stellar flares using the Dark Energy Camera as part of the Deeper, Wider, Faster programme. The data were collected via continuous 20-s cadence g -band imaging and we identify 19 914 sources with precise distances from Gaia DR2 within 12, ∼3 deg 2, fields over a range of Galactic latitudes. An average of ∼74 min is spent on each field per visit. All light curves were accessed through a novel unsupervised machine learning techniques designed for anomaly detection. We identify 96 flare events occurring across 80 stars, the majority of which are M dwarfs. Integrated flare energies range from ∼10 31 –10 37 erg, with a proportional relationship existing between increased flare energy with increased distance from the Galactic plane, representative of stellar age leading to declining yet more energetic flare events. In agreement with previous studies we observe an increase in flaring fraction from M0 to M6 spectral types. Furthermore, we find a decrease in the flaring fraction of stars as vertical distance from the galactic plane is increased, with a steep decline present around ∼100 pc. We find that $\sim 70{{\ \rm per\ cent}}$ of identified flares occur on short time-scales of <8 min. Finally, we present our associated flare rates, finding a volumetric rate of 2.9 ± 0.3 × 10 −6 flares pc −3 h −1 .