Image Details
Caption: Figure 2.
(Top left) Resolve spectra in the 2.0–10.0 keV energy band for the cold front (CF_IN, black) and central (Center, red) pointings. The best-fit models are overlaid on each spectrum together with NXB models. (Top right) Zoom-in of the Resolve spectra in the 6.2–6.7 keV energy band. Data are binned by 2 eV for display purposes. (Bottom) The spectra in regions a–g used for the SSM analysis in the 6.2–6.7 keV energy band. Each colored curve shows the modeled emission from the corresponding sky region: region a (red), b (orange), c (blue), d (green), e (magenta), f (cyan), and g (light gray). The spectrum of region a is also shown with the sum of all models (black) except for the region a model, highlighting the blueshifted contribution of region a relative to the others.
© 2025. The Author(s). Published by the American Astronomical Society.