Synthetic fluxes at 1 au from GJ 3470 in the FUV and two EUV bands as a function of time. We distinguish the fluxes calculated with the EMD model of GJ 3470 alone (solid lines) and the EMD model of the combined GJ 3470 and AD Leo (dotted lines). Numbers over the flare peaks indicate the maximum-to-minimum ratio of the curves in each band. We note that variations in X-rays (5–100 Å, not shown here) are limited to two main values in the case of the combined EMD (5.7 × 10²⁷ erg s⁻¹, quiescent; 1.8 × 10²⁸ erg s⁻¹, flares), while it is almost constant for all intervals in the EMD of GJ 3470 alone (2.3 × 10²⁷).