Index: trunk/MagicSoft/GRB-Proposal/Timing.tex
===================================================================
--- trunk/MagicSoft/GRB-Proposal/Timing.tex	(revision 6269)
+++ trunk/MagicSoft/GRB-Proposal/Timing.tex	(revision 6270)
@@ -20,9 +20,13 @@
 \item Regarding the fireball model~\cite{REES1,REES2},
 two efficient mechanisms are available for the generation of VHE photons~\cite{DERISHEV}. 
-(1) The prompt emission of $\sim$100\,GeV photons is expected before and during the keV-MeV peak. 
+
+\begin{enumerate}
+\item The prompt emission of $\sim$100\,GeV photons is expected before and during the keV-MeV peak. 
 This emission should have their highest luminosity together with the main GRB peak. 
-(2) VHE photons generated due to inverse Compton (IC) scattering in relativistic shocks 
+\item VHE photons generated due to inverse Compton (IC) scattering in relativistic shocks 
 are strongly absorbed by infrared background radiation and 
 cannot be observed from cosmological distances. 
+\end{enumerate}
+
 With the presence of a dense ambient medium close to the GRB, 
 the UHE photons will be reprocessed into a softer spectral range. 
@@ -99,3 +103,4 @@
 %%% mode: latex
 %%% TeX-master: "GRB_proposal_2005"
+%%% TeX-master: "Timing"
 %%% End: