% Please use the skeleton file you have received in the
% invitation-to-submit email, where your data are already
% filled in. Otherwise please make sure you insert your
% data according to the instructions in PoSauthmanual.pdf
\documentclass{PoS}

\title{Spectral classification and variation of Fermi GRBs
}

\ShortTitle{}

\author{\speaker{Istvan Racz}\\
        RCAES HAS Konkoly Observatory
 \\
        E-mail: \email{racz@complex.elte.hu
}}

%\author{Another Author\\
%        Affiliation\\
%        E-mail: \email{...}}

\abstract{
  The Fermi GBM catalog contains general physical quantities of the observed objects and also estimated parameters (peak energy, spectral indices, intensity) from four fitted spectral models (Band, smoothly broken power law, Comptonized, power law) for the peak flux and the fluence. We studied the nature of the errors of the peak flux, the fluence, and duration parameters. We have found a linear correlation between the logarithm of the measured quantities and their error bars. We interpret our results as an indication, that the peak flux, fluence and duration follow a Poissonic distribution.
}

\FullConference{7th Fermi Symposium 2017\\
		15-20 October 2017\\
		Garmisch-Partenkirchen, Germany}


\begin{document}

%\section{...}

%\begin{thebibliography}{99}
%\bibitem{...}
%....
%\end{thebibliography}

\end{document}
