Table 1: Maximum redshift of detection by AGILE and GLAST as a function of the fireball Lorentz factor $\Gamma $, the prompt temporal variability $t_{\rm v}$, and the instrumental integration time $T_{\rm int}$. The other parameters are fixed as L52=1.0, $\epsilon _{\rm e}=0.45$, $\epsilon _B=0.1$, and p=2.5. We also report the peak energies $E_{\rm p}$ of the synchrotron prompt emission and the cutoff energies $E_{\rm cut}$ of the relative SSC component.
Satellite $\Gamma $ $t_{\rm v}$ $T_{\rm int}$ $z_{\rm max}$ $E_{\rm p}$ $E_{\rm cut}$
    [ms] [s]   [keV] [MeV]

AGILE		 600 1 10 1.8 7.78 $5.4\times 10^3$
GLAST 600 1 10 3.0 5.44 $3.8\times 10^3$
AGILE 600 1 50 3.2 5.18 $3.6\times 10^3$
GLAST 600 1 50 5.5 3.35 $2.3\times 10^3$
AGILE 600 10 10 3.0 0.54 $3.8\times 10^4$
GLAST 600 10 10 4.0 0.44 $3\times 10^4$
AGILE 600 10 50 6.5 0.29 $2\times 10^4$
GLAST 600 10 50 7.0 0.27 $1.9\times 10^4$
AGILE 200 10 10 1.5 7.8 127.9
GLAST 200 10 10 2.0 6.5 106.6
AGILE 200 10 50 2.0 6.5 106.6
GLAST 200 10 50 2.0 6.5 106.6


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