\bibitem{grb161219B17bcpt}Kann, D. A., et al. 2017, ApJ, 841, 36K

\bibitem{HHV13}Hartmann, D., Hakkila, J., \& Vilhu, O. 2013, GCN Circ. 15136

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\begin{bf} Figures \end{bf}

%% Fig 1 \begin{figure} \epsscale{0.7}

\plotone{f1.eps}

\caption{Light curves of GRB 161219B in 8–1000\,keV band measured by different satellites: Konus-Wind (depicted by black circles; Golenetskii et al. 2016), Swift-XRT (green circles; Evans et al. 2016), INTEGRAL-IBIS (blue circles; Gotz et al. 2016), Suzaku-WAM (purple circles; Sakamoto et al. 2016b), and INTEGRAL-JEM-X (red inverted triangles; Sakamoto et al. 2016a). The light curve of the prompt emission measured in MeV range by Fermi-GBM is also shown (black circles) overlain by two dashed vertical lines which enclose the time interval of a possible extended emission. } \end{figure}

%% Fig 2 \begin{figure} \epsscale{0.7}

\plotone{f2.eps}

\caption{Time resolved spectroscopic analysis results for two intervals of the extended emission of GRB 161219B: Time 1 (First box in Fig. 1) and Time 2 (Second box in Fig. 1). The measured flux spectra are depicted in black circles and the best fit model spectra are depicted in red lines (see the text for details). } \end{figure}

%% Fig 3 \begin{figure} \epsscale{0.7}

\plotone{f3.eps}

\caption{Time resolved spectroscopic analysis results of a possible extended emission of GRB 170112A in different energy intervals. The time intervals are divided into three (a), four (b), and five (c) bins labeled from T1 to T5 based on their temporal evolution. The measured flux spectra are depicted in black circles and the best fit model spectra are depicted in red lines (see the text for details). } \end{figure}

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