Neutrinos from Cosmic Accelerators including Magnetic Field and Flavor Effects
Figure 12
(a) Distribution of 10 000 bursts as a function of redshift (histograms) and relative contribution of the individual GRBs (solid curves). The dashed curve shows the exact distribution function. Here it is assumed that the GRBs follow the star formation rate from Hopkins and Beacom [117] with the correction from Kistler et al. [118]. (b) Probability that the quasi-diffuse flux extrapolated from a low statistics sample with bursts is larger than a certain fraction of the diffuse limit (see legend for different values of ). This function corresponds to (one minus) the cumulative distribution function of the probability density, figure taken from [30].
