Table 3: List of GRB afterglow fluxes extrapolated or interpolated 11 and 12 h after the burst from their spectral and temporal parameters (assuming there is no evolution of these parameters). These two times are chosen to match the works by De Pasquale et al. (2006) and Berger et al. (2005) about Beppo-SAX and SWIFT respectively. We have separated the Chandra Grating ( top), Chandra Imaging ( center) and XMM-Newton ( bottom) samples due to their different observation times, and have removed GRB 030329 due to its very late XMM-Newton observation.
GRB Name Flux Flux
  11 h 12 h
  (erg cm-2 s-1) (erg cm-2 s-1)
GRB 020405 $7.1 \pm 0.3 \times 10^{-12}$ $6.2 \pm 0.3 \times 10^{-12}$
GRB 020813 $3.93\pm0.08 \times 10^{-12}$ $3.48\pm0.07 \times 10^{-12}$
GRB 021004 $8.4 \pm 0.5 \times 10^{-13}$ $7.6 \pm 0.4 \times 10^{-13}$
GRB 030328 $2.9 \pm 0.2 \times 10^{-13}$ $2.5 \pm 0.2 \times 10^{-13}$
GRB 000210 $6.7 \pm 0.3 \times 10^{-13}$ $6.0 \pm 0.3 \times 10^{-13}$
GRB 000926 $3.1 \pm 0.2 \times 10^{-12}$ $2.7 \pm 0.2 \times 10^{-12}$
GRB 011030 $1.8 \pm 0.5 \times 10^{-11}$ $1.6 \pm 0.4 \times 10^{-11}$
GRB 030226 $1.35\pm0.08 \times 10^{-12}$ $1.10\pm0.07 \times 10^{-12}$
GRB 001025A $1.2 \pm 0.2 \times 10^{-13}$ $1.1 \pm 0.2 \times 10^{-13}$
GRB 011211 $1.72\pm0.05 \times 10^{-13}$ $1.46\pm0.05 \times 10^{-13}$
GRB 020322 $4.2 \pm 0.1 \times 10^{-13}$ $3.8 \pm 0.1 \times 10^{-13}$
GRB 031203 $4.5 \pm 0.1 \times 10^{-13}$ $4.3 \pm 0.1 \times 10^{-13}$
GRB 040106 $9.9 \pm 0.2 \times 10^{-13}$ $9.0 \pm 0.2 \times 10^{-13}$
GRB 040223 $2.3 \pm 0.2 \times 10^{-13}$ $2.2 \pm 0.2 \times 10^{-13}$
GRB 040827 $1.40\pm0.05 \times 10^{-13}$ $1.26\pm0.05 \times 10^{-13}$

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