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Table 1:

Fermi long GRBs with redshift.

GRB
z $\alpha $ $E_{\rm peak}$ $\beta$ P F-6 Range GCN $L_{\rm iso,52}$ $E_{\rm iso,52}$
      keV   ph/s/cm2 erg/cm2 keV number erg/s erg
080810.549 3.35 $-0.91\pm0.12$ $313.5\pm 3.6$   $1.85\pm0.16$ $6.9\pm0 .5$ 50-300 8100 7.84 33.2
080905.705 2.374 $-1.75 \pm 0.12$     $0.21\pm 0.02$ $0.04\pm 0.003$ 20-1000 8205    
080916.406 0.689 $-0.9\pm 0.1$ $109 \pm 9$   $4.5\pm 0.7$ $15\pm 5$ 25-1000 8263 0.142 2.25
080916.009* 4.35 $-0.91\pm 0.02$ $424\pm 24$ $-2.08\pm 0.06$ 1.2e-5** 190 8-30000 8278 190 563
080928.628 1.692 $-1.80\pm 0.08$       $1.5\pm 0.1$ 50-300 8316    
081007 0.529 $-1.4 \pm 0.4$ $40\pm 10$   $2.2\pm 0.2$ $1.2 \pm 0.1$ 25-900 8369 0.041 0.172
081222.204 2.77 $-0.55 \pm 0.07$ $134\pm 9$ $-2.10\pm 0.06$ $14.8\pm1.4$ $13.5\pm 0.8$ 8-1000 8715 20.6 35.4
090323.002* 3.57 $-0.89\pm 0.03$ $697\pm 51$   $12.3\pm 0.4$ $100\pm 1$ 8-1000 9035 47.2 338
090328.401* 0.736 $-0.93 \pm 0.02$ $653\pm 45$ $-2.2\pm 0.1$ $18.5\pm 0.5$ $80.9 \pm 1$ 8-1000 9057 1.96 21.2
090423.330 8.2 $-0.77\pm 0.35$ $82\pm 15$   $3.3 \pm 0.5$ $1.1\pm 0.3$ 8-1000 9229 18.8 10.2
090424.592 0.544 $-0.90 \pm 0.02$ $177\pm 3$ $ -2.9\pm 0.1$ $137\pm 5$ $52 \pm 1$ 8-1000 9230 2.12 4.48
090618.353 0.54 $-1.26\pm 0.04$ $155.5\pm 11$ $-2.5\pm 0.25$ $73.4\pm 2.0$ $270\pm 6$ 8-1000 9535 1.0 25.7

Notes. (*) GRBs with a detection also in the LAT instrument on-board Fermi. (**) The energy peak flux of GRB 080916.009 is in the 20 keV-10 MeV range, from Golenetskii et al. (2008a).


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