Image Details
Caption: Figure 2.
Spectral fit of eRASSU J060839.5–704014 using NICER (left) and EP-FXT (right) modeled with absorbed blackbody emission. The background contribution for NICER was modeled with SCORPEON. The colored bands enclose 99% posterior uncertainties on the model at each energy. The spectra are rebinned for plotting purposes.
© 2026. The Author(s). Published by the American Astronomical Society.