Fully deprojected temperature, density, cooling time (t_cool), and entropy profiles. The dotted horizontal lines in panels (c) and (d) show the thresholds for cooling time of 5 × 10⁸ yr and for entropy of 30 keV cm², respectively. Note that all sources satisfy both thresholds, as was the case for the projected profiles (see Figure 1). In panel (d) we show the overall best fitting power-law model to the inner entropy profiles of a sample of 66 nearby clusters presented by Panagoulia et al. (2014) and a standard cluster entropy profile with scaling K ∝ r^1.1 as expected from gravity alone (e.g., Tozzi & Norman 2001; Voit et al. 2005). Note that the normalization of this latter power law is adjusted to match our profiles.