Image Details
Caption: Figure 4.
Upper panel: the unabsorbed X-ray flux in the full XRISM/Resolve band (2.2–17.4 keV), as measured via Swift/XRT monitoring observations. Lower panel: the flux of the BLR component of the Fe Kα emission lines, as measured via joint fits to Resolve and Xtend spectra.
© 2026. The Author(s). Published by the American Astronomical Society.