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\title{On the Connection of Gamma-Ray Bursts and X-Ray Flashes
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\author{\speaker{Jakub  \v{R}\'{\i}pa}\\
        formerly: National Taiwan University / LeCosPA\\
        No.1, Sec.4, Roosevelt Road, Taipei 10617, Taiwan (R.O.C)\\
        E-mail: \email{ripa.jakub@gmail.com}}

\author{Attila M\'esz\'aros\\
        Charles University,\\
        Faculty of Mathematics and Physics, Astronomical Institute,\\
        V Hole\v{s}ovi\v{c}k\'ach 2, 180 00 Prague 8, Czech Republic\\
        E-mail: \email{meszaros@cesnet.cz}}

\abstract{
  Classification of gamma-ray bursts (GRBs) into groups has been intensively studied by various statistical tests since 1998. It has been suggested that next to the groups of short/hard and long/soft GRBs there could be another class of intermediate durations. For the Swift/BAT database Veres et al. 2010 (ApJ, 725, 1955) it was found that the intermediate-duration bursts might be related to X-ray flashes (XRFs). On the other hand,  \v{R}\'{\i}pa and M\'esz\'aros 2016 (Ap\&SS, 361, 370) and  \v{R}\'{\i}pa et al. 2012 (ApJ, 756, 44) found that the intermediate-duration GRBs in the RHESSI database are spectrally too hard to be given by XRFs. Also, in the BATSE database the intermediate-duration GRBs can be only partly populated by XRFs. The key ideas of the  \v{R}\'{\i}pa and M\'esz\'aros 2016 (Ap\&SS, 361, 370) article are summarized in this poster.
}

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


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