Image Details
Caption: Figure 3.
Amplitude–energy and amplitude–duration relations for JWST flares. (a) Relationship between normalized Hα flare amplitude and inferred ETESS and (b) between amplitude and flare duration (FWHM) for the NIRISS and NIRSpec/PRISM flare samples. Dashed lines show linear fits in log–log space. The energy–amplitude mapping is steep and relatively tight, whereas the duration–amplitude trend is weaker and more scattered; we therefore scale injected flares in amplitude only for the injection–recovery test.
© 2026. The Author(s). Published by the American Astronomical Society.