VizieR Online Data Catalog: K2 ultracool dwarfs survey. III. M6-L0 flares (Paudel+, 2018)

All the 10 targets listed in Table 1 were observed by Kepler K2 in various campaigns (see the campaign number in Table 1) in both long-cadence mode (~30 min) and short-cadence mode (~1 min). We used short-cadence data to study white light flares (WLFs) on all of our targets.

(3 data files).