Open Access
Fig. 32
Download original image
Example spectra having χ2/d.o.f of 1.50 and 1.70, respectively. They are commonly found near the Galactic plane, towards the inner part of the Galaxy and the base of the eROSITA bubbles. The models usually cannot predict the spectrum between ~0.7–1 keV well.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.