Fig. 4 | Nature Communications

Fig. 4

From: The photospheric origin of the Yonetoku relation in gamma-ray bursts

Fig. 4

Relation between time-resolved spectral peak energy Ep and peak luminosity Lp. Same as Fig. 3, but for a spectral peak energy and peak luminosity computed in five time intervals of Δt = 10 s successively taken within an observer time tobs = 50 s. The error bars of the observational data indicate 1-σ standard error for both Ep and Lp