\begin{table}%t1
\caption{\label{catalog}The 25 GRBs with known redshift and measured \epi\ added to the sample of 
\citet{Amati08} in our analysis of the \epeiso~correlation, providing a total of~95~GRBs.}
\par
\small%\centerline
 {
\begin{tabular}{lccccc}
\hline \hline \noalign{\smallskip}
GRB & $z$$^a$ &  \epi  & \eiso$^b$ & Instrument$^c$ & Ref.$^d$ \\
 & & [\rm keV] & [{\rm 10$^{52}$ erg}] \\
\hline
  020127  & 1.9  & 290 $\pm$ 100  &  3.5 $\pm$ 0.1  & HET & (1)  \\
  071003  & 1.604  & 2077 $\pm$ 286  &  36 $\pm$ 4  & KW & (2)  \\
  080413  & 2.433  & 584 $\pm$ 180  &  8.1 $\pm$ 2.0  & BAT/WAM & (3)  \\
  080413B & 1.10  & 150 $\pm$ 30  &  2.4 $\pm$ 0.3  & BAT & (4)  \\
  080514B & 1.8  & 627 $\pm$ 65  &  17 $\pm$ 4  & KW & (5)  \\
  080603B & 2.69   & 376 $\pm$ 100  &  11 $\pm$ 1  & KW & (6)  \\
  080605  & 1.6398  & 650 $\pm$ 55  &  24 $\pm$ 2  & KW & (7)  \\
  080607  & 3.036  & 1691 $\pm$ 226  &  188 $\pm$ 10  & KW & (8)  \\
  080721  & 2.591  & 1741 $\pm$ 227  &  126 $\pm$ 22  & KW & (9)  \\
  080810  & 3.35  & 1470 $\pm$ 180  &  45 $\pm$ 5  & GBM & (10)  \\
  080913  & 6.695  & 710 $\pm$ 350  &  8.6 $\pm$ 2.5  & BAT/KW & (11)  \\
  080916  & 0.689  & 184 $\pm$ 18  &  1.0 $\pm$ 0.1  & BAT/GBM$^e$ & (12)  \\
  081007  & 0.5295  & 61 $\pm$ 15 & 0.16 $\pm$ 0.03 & GBM & (13)  \\
  081008  & 1.9685  & 261 $\pm$ 52  &  9.5 $\pm$ 0.9  & BAT & (14)  \\
  081028  & 3.038  & 234 $\pm$ 93  &  17 $\pm$ 2  & BAT & (15)  \\
  081118  & 2.58  & 147 $\pm$ 14  &  4.3 $\pm$ 0.9  & BAT/GBM$^{\it e}$
   & (16)  \\
  081121  & 2.512  & 871 $\pm$ 123  &  26 $\pm$ 5  & KW & (17)  \\
  081222  & 2.77  & 505 $\pm$ 34  &  30 $\pm$ 3  & GBM & (18)  \\
  090102  & 1.547  & 1149 $\pm$ 166 & 22 $\pm$ 4 & KW & (19)  \\
  090328  & 0.736  & 1028 $\pm$ 312 & 13 $\pm$ 3 & KW & (20)  \\
  090418  & 1.608  & 1567 $\pm$ 384 & 16 $\pm$ 4  & BAT/KW & (21)  \\
  090423  & 8.1   & 491 $\pm$ 200 & 11 $\pm$ 3 & GBM & (22)  \\
  090424  & 0.544  & 273 $\pm$ 50  &  4.6 $\pm$ 0.9  & GBM & (23)  \\
\hline
  080916C  & 4.35  & 2646 $\pm$ 566 &380 $\pm$ 80 & GBM/KW & (24)  \\
  090323  & 3.57  & 1901 $\pm$ 343 & 410 $\pm$ 50 & KW & (24)  \\
\hline
\end{tabular}}
\medskip
$^a$ Taken from the GRB table by J. Greiner and references therein (\url{http://www.mpe.mpg.de/jcg/grbgen.html}).  \\
$^b$ Computed in the 1--10~000~keV cosmological rest-frame by assuming a standard $\Lambda$CDM~cosmology with $H_{0}= 70$~km~s$^{-1}$~Mpc$^{-1}$, \omegam~= 0.27 and \omegal~= 0.73.  \\
$^c$ Instrument(s) that provided the spectral parameters and fluence used for the computation of \epi\ and \eiso: HET~= HETE--2; BAT~= \swift/BAT; KW~= \konus/WIND; WAM~= \suz/WAM; GBM~= \fermi/GBM. \\
$^d$ References for spectral parameters and fluence: (1) \citet{Sakamoto05}; 
(2)~\citet{Golenetskii07}; (3)~\citet{Ohno08}; (4)~\citet{Barthelmy08a}; (5)~\citet{Golenetskii08a}; (6)~\citet{Golenetskii08b}; (7)~\citet{Golenetskii08c}; (8)~\citet{Golenetskii08d}; (9)~\citet{Golenetskii08e};
(10)~\citet{Meegan08};
(11)~\citet{Palshin08};
(12)~\citet{Bissaldi08a} and \citet{Baumgartner08};
(13)~\citet{Bissaldi08b};
(14)~\citet{Palmer08a};
(15)~\citet{Barthelmy08b};
(16)~\citet{Palmer08b} and~\citet{Bhat08};
(17)~\citet{Golenetskii08g};
(18)~\citet{Bissaldi08c};
(19)~\citet{Golenetskii09a};
(20)~\citet{Golenetskii09c};
(21)~\citet{Palshin09};
(22)~\citet{Kienlin09};
(23)~\citet{Connaughton09}; (24)~see text.  \\
$^e$ Spectral parameters from \fermi{}/GBM and fluence from \swift/BAT.
\end{table}