Spatially resolved morphological and thermodynamic analysis of PSZ2 G282.28+49.94. Top left panel: same as in Fig. 2, with the position of the X-ray peaks highlighted by the magenta points and the iso-contours derived from the wavelet-cleaned image in the top right panel. Top right panel: wavelet-cleaned image in the [0.5–2.5] keV band centred on the central part of the cluster. The white circle encompasses $R_{500}^{{\text{Y}}_{\text{X}}}$. The two crosses identify the position of BCG1 and BCG2 described in Sect. 3.2. The cyan contours identify the iso-levels of the spectroscopic galaxy members of PSZ2 G282.28+49.94. The map is in unit of counts. Bottom left panel: offset view of the extended emissions in the E sector highlighted by the magenta squares, as in Fig. 2. The E emission is interacting with the main cluster, being at the same redshift. The SE is associated with a foreground group emission at z ~ 0.17 (see Sect. 3.4 for more details). Bottom right panel: Temperature map of PSZ2 G282.28+49.94. The white lines identify the iso-contours derived from the wavelet-cleaned map shown in the top right panel. The dotted black circles identify the three regions within which we extracted the spectra to derive the spectroscopic temperature, whose co-ordinates and radius are reported in Table 2. The units of the colour bar are keV.