Extended Data Figure 3: Elemental abundances calculated with different model assumptions.
From: Solar abundance ratios of the iron-peak elements in the Perseus cluster
‘A’ and ‘S’ indicate the results obtained using the atomic databases AtomDB v.3.0.8 and SPEX v.3.03, respectively, and ‘S′’ represents an old atomic model (SPEX v.2.05, which does not contain Cr and Mn line data). Numerical designations are as follows: ‘1’, one-temperature fit with the Fe xxv resonance-scattering effect; ‘2’, one-temperature fit without the resonance-scattering effect; ‘3’, two-temperature fit with the resonance-scattering effect; ‘4’, two-temperature fit without the resonance-scattering effect. The error bars correspond to the 1σ confidence level.
