Extended Data Fig. 2: Comparison of the XRISM/Resolve spectrum and Chandra/HETG first order spectrum around the iron Kα line of Circinus.
From: Accurate determination of chemical abundances near a supermassive black hole
The former (this work) is binned with 0.5 eV. The latter is adopted from Uematsu et al.20 and is binned with 9 eV. The error bars denote the 1σ confidence limits in photon statistics.
