Upper panels: the projected temperature profiles of the six clusters of our sample. For the first four objects, Swift XRT measurements (black points) are compared with XMM-Newton (blue points) Snowden et al. (2008). In the Coma plot we also report the BeppoSAX numbers from De Grandi & Molendi (2002). In the Abell 2029 and Abell 1795 plots we report the Chandra measurements from Vikhlinin et al. (2006). In the PKS0745-19 we report the Suzaku points (George et al. 2009). In the case of SWJ1557+35 and SWJ0847+13 we compare measurements obtained with locally evaluated and modeled background. Middle panels: fluxes in the 0.3−10. keV band in cgs deg^-2 units compared with XMM-Newton values from Snowden et al. (2008), in the first four cases, and with the value after local background subtraction in the remaining two. Lower panels: for each extraction region we plot the relative value of the 0.5−2.0 keV band flux for the cluster (black), XRB (green) and NXB (red).