Example of flares detected with the finding algorithm, described in Appendix A.3, shown for TESS (left) and COS (right) observations of Karmn J07446+035 (YZ CMi). The TESS flare, found in Sector 34, the fast (20 s) cadence observation has an ED = 978.54 s and the total energy in TESS bandpass of ≈2.38 × 10³³ erg. Applying a correction factor of 0.19 for the TESS CCD response and assuming a blackbody model of 9000 K (Petrucci et al. 2024; Howard & MacGregor 2022) to calculate the bolometric energy of the flare, we obtained E_bol ≈ 1.3  ×  10³⁴ erg, consistent with Namizaki et al. (2023). The right panel shows a flare in COS-HST observed 2024-04-12 with starting time 08:36:35.26, with ED = 1836.18 s and a total energy in G130M range of ≈2.70 × 10²⁹ erg.