Image Details
Caption: Figure 8.
By taking fits across the time series of each energy, as shown in (a) for 1.74 keV, we generate a spectrum as shown in (b) by extracting the peak flux from the fit. The total fit is shown in black, with the spectral components added as shown in the legend. The fit has residuals shown below to further illustrate fit quality.
© 2026. The Author(s). Published by the American Astronomical Society.