Image Details
Caption: Figure 11.
Five flares of L 98-59 seen in TESS 2 minutes cadence data. The flares vary in peak fractional change in stellar brightness from 0.2% to 3.5%. There is also one complex flare that shows multiple peaks. The green curves are flare models with uncertainty regions inferred using an MCMC method.
© 2025. The Author(s). Published by the American Astronomical Society.