Fig. 3.

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Left column: Evolution of the flux in 0.3−150 keV energy band (top), evolution of νc (middle), and νc as a function of F0.3 − 150 keV (bottom), assuming a synchrotron spectral model. Right column: Evolution of the flux in 0.3−150 keV energy band (top), evolution of Ep (middle), and Ep as a function of F0.3 − 150 keV (bottom), assuming a sBPL spectral model. Each color refers to a different GRB. Error bars represent 1σ uncertainties, while arrows represent 68% upper limits.
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