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Fig. 6


Calibrated GRB Hubble diagram (black filled diamond) up to very high values of redshift, as constructed by applying the local regression technique with the Reichart likelihood: we show overplotted the behavior of the theoretical distance modulus μ(z) = 25 + 5log dL(z) corresponding to the favored fitted CPL model (red line), with w0 = −0.29, w1 = −0.12, h = 0.74, Ωm = 0.24, and the standard ΛCDM model (gray line) with Ωm = 0.33, and h = 0.74. They are defined by Eqs. (12) and (21). The blue filled points at lower redshift are the SNIa data.

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