Fig. 4.
Left: bolometric flare emitted energy, estimated from the Spitzer lightcurves assuming a 104 K black body spectrum, EIR, vs. EX the energy emitted in the 0.5–8.0 keV band. Symbols and lines as in Fig. 3/5, with the addition of blue circles, which indicate flares from Class I sources. Right: same as the plot on the left, but for peak luminosities instead of energies.
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