All Figures

$\begin{figure} \par\resizebox{18cm}{!} {\hspace{0mm} \includegraphics{7966fg01.e... ...aphics{7966fg02.eps} \hspace{0mm} \includegraphics{7966fg03.eps} } \end{figure}$ Figure 1: The surface brightness profiles combined MOS1, MOS2, and pn cameras obtained using different backgrounds: a) the background of A. Read, b) the background of Nevalainen, and c) the background model from observation data. The solid line is the best-fit $\beta$ -model.
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In the text

$\begin{figure} \par\resizebox{8.8cm}{!} { \hspace{0mm} \includegraphics{7966f... ...hics{7966fg05.eps} \hspace{0mm} \includegraphics{7966fg06.eps} } \end{figure}$ Figure 2: The combined (MOS1, MOS2, pn) surface brightness profiles in the external region obtained using: a) the background of A. Read, b) the background of J. Nevalainen, c) the background modelling from corresponding observation data. The solid line is the best-fit $\beta$ -model.
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In the text

$\begin{figure} \par\includegraphics[width=5.9cm,angle=270, trim=45 0 15 0, clip, keepaspectratio]{7966fg07.ps} \end{figure}$ Figure 3: CL0016+16 extracted spectra in the region $5\hbox {$^\prime $ }$ from the XMM-Newton data. Black, red, green points are the data from the corresponding EPIC/ MOS1, MOS2, and pn data. The solid lines show the best fit of the isothermal model with kT = 8.81 keV and abundance of 0.18 solar units.
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In the text

$\begin{figure} \par\includegraphics[width=7.6cm, keepaspectratio]{7966fg08.ps} \end{figure}$ Figure 4: The obtained total temperature profile of CL0016+16. The solid points and line are the obtained temperatures and the fitting of the temperature profile function. The thin points and dotted line are the obtained temperatures and the temperature profile function of Kotov & Vikhlinin (2005).
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In the text

$\begin{figure} \par\includegraphics[width=7.6cm,keepaspectratio]{7966fg09.ps} \end{figure}$ Figure 5: a) The X-ray emission from EPIC (MOS1, MOS2, and pn cameras) in the energy band 0.3-4.5 keV. b) The temperature map obtained by wavelet algorithm described in Bourdin et al. (2004).
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In the text

$\begin{figure} \par\includegraphics[width=7.6cm, keepaspectratio]{7966fg10.ps} \end{figure}$ Figure 6: The temperature map with chosen regions and sectors. The white contours illustrate the chosen regions from which spectra were extracted. The regions were defined on the basis of temperature map. The green contours are the sectors chosen, for extracting the spectra for four temperature profiles.
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In the text

$\begin{figure} \par\mbox{\includegraphics[width=4cm]{7966fg11.ps}\hspace{2mm} \includegraphics[width=4cm]{7966fg12.ps} } \end{figure}$ Figure 7: The temperature profiles in different directions. The solid points are the total temperature profile. The dotted points are the obtained temperature profiles from sectors: a) the "hot'' temperature profiles (the SE and NW directions) b) the "cold'' temperature profiles (the SW and NE directions) correspondingly. The "cold'' temperature profile (SW) in panel b) displays a local peak because of the offset of the temperature peak visible in Fig. 6.
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In the text

$\begin{figure} \par\includegraphics[width=7.6cm,keepaspectratio]{7966fg13.eps} \end{figure}$ Figure 8: The surface brightness profiles in different directions. The solid line is the best fit of the total radial profile.
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In the text

$\begin{figure} \par\includegraphics[width=7.6cm,keepaspectratio]{7966fg14.ps} \end{figure}$ Figure 9: The integrated total mass profile of CL0016+16. a) The bold solid line showing the total mass profile was obtained using the total temperature profile. The dot-dashed line is the total mass profile obtained using constant temperature. b) The bold solid line is the total mass profile obtained using the total temperature profile. c) The solid line is the total mass profile obtained using the "cold'' temperature profiles. d) The dotted line is the total mass profile obtained using the "hot'' temperature profiles.
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In the text

$\begin{figure} \par\resizebox{18cm}{!} {\hspace{0mm} \includegraphics{7966fg15.ps}} \end{figure}$ Figure 10: a) The X-ray emission from the XMM-Newton data. b) The X-ray residual from the XMM-Newton data in the cluster centre, was obtained with the help of 2D $\beta$ -model. c) The obtained X-ray residual from the Chandra data.
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In the text

$\begin{figure} \par\resizebox{8.8cm}{!} {\includegraphics{7966fg16.ps}} \end{figure}$ Figure 11: The scaled emission measure (ScEM) profiles. The dotted lines are the ScEM profiles of the nearby clusters. The bold solid line shows the ScEM profile of CL0016+16. The radius is normalised to R₂₀₀.
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In the text

$\begin{figure} \par\includegraphics[width=7.6 cm,keepaspectratio]{7966fg17.eps} \end{figure}$ Figure A.1: The surface brightness profile for a similar cluster to CL0016+16 obtained from the Hydro N-body cosmology simulations.

In the text

$\begin{figure} \par\resizebox{18cm}{!} {\hspace{0mm} \includegraphics{7966fg01.e... ...aphics{7966fg02.eps} \hspace{0mm} \includegraphics{7966fg03.eps} } \end{figure}$	Figure 1: The surface brightness profiles combined MOS1, MOS2, and pn cameras obtained using different backgrounds: a) the background of A. Read, b) the background of Nevalainen, and c) the background model from observation data. The solid line is the best-fit $\beta$ -model.
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$\begin{figure} \par\resizebox{8.8cm}{!} { \hspace{0mm} \includegraphics{7966f... ...hics{7966fg05.eps} \hspace{0mm} \includegraphics{7966fg06.eps} } \end{figure}$	Figure 2: The combined (MOS1, MOS2, pn) surface brightness profiles in the external region obtained using: a) the background of A. Read, b) the background of J. Nevalainen, c) the background modelling from corresponding observation data. The solid line is the best-fit $\beta$ -model.
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$\begin{figure} \par\includegraphics[width=5.9cm,angle=270, trim=45 0 15 0, clip, keepaspectratio]{7966fg07.ps} \end{figure}$	Figure 3: CL0016+16 extracted spectra in the region $5\hbox {$^\prime $ }$ from the XMM-Newton data. Black, red, green points are the data from the corresponding EPIC/ MOS1, MOS2, and pn data. The solid lines show the best fit of the isothermal model with kT = 8.81 keV and abundance of 0.18 solar units.
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$\begin{figure} \par\includegraphics[width=7.6cm, keepaspectratio]{7966fg08.ps} \end{figure}$	Figure 4: The obtained total temperature profile of CL0016+16. The solid points and line are the obtained temperatures and the fitting of the temperature profile function. The thin points and dotted line are the obtained temperatures and the temperature profile function of Kotov & Vikhlinin (2005).
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$\begin{figure} \par\includegraphics[width=7.6cm,keepaspectratio]{7966fg09.ps} \end{figure}$	Figure 5: a) The X-ray emission from EPIC (MOS1, MOS2, and pn cameras) in the energy band 0.3-4.5 keV. b) The temperature map obtained by wavelet algorithm described in Bourdin et al. (2004).
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$\begin{figure} \par\includegraphics[width=7.6cm, keepaspectratio]{7966fg10.ps} \end{figure}$	Figure 6: The temperature map with chosen regions and sectors. The white contours illustrate the chosen regions from which spectra were extracted. The regions were defined on the basis of temperature map. The green contours are the sectors chosen, for extracting the spectra for four temperature profiles.
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$\begin{figure} \par\includegraphics[width=7.6cm,keepaspectratio]{7966fg13.eps} \end{figure}$	Figure 8: The surface brightness profiles in different directions. The solid line is the best fit of the total radial profile.
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$\begin{figure} \par\resizebox{18cm}{!} {\hspace{0mm} \includegraphics{7966fg15.ps}} \end{figure}$	Figure 10: a) The X-ray emission from the XMM-Newton data. b) The X-ray residual from the XMM-Newton data in the cluster centre, was obtained with the help of 2D $\beta$ -model. c) The obtained X-ray residual from the Chandra data.
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$\begin{figure} \par\resizebox{8.8cm}{!} {\includegraphics{7966fg16.ps}} \end{figure}$	Figure 11: The scaled emission measure (ScEM) profiles. The dotted lines are the ScEM profiles of the nearby clusters. The bold solid line shows the ScEM profile of CL0016+16. The radius is normalised to R₂₀₀.
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