Fig. 2 | Nature Communications

Fig. 2

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

Fig. 2

Light curves and time integrated spectra. a Light curves up to observer time tobs = 110 s. b Time integrated spectra constructed by averaging over the duration tdur = 110 s. Line color indicates jet power, with red, green, and blue showing the cases of Lj = 1049, 1050, and 1051 erg s−1, respectively. For each model, we show results for three different viewing angles: θobs = 0° (solid line), 5° (dashed), and 10° (dotted). Note that, although high-energy photons suffer from low statistics, this does not affect the evaluation of the overall luminosity or the spectral peak energy