Fig. A.3.
Left panel: Chandra High Resolution Camera (HRC) observation of HE 1353−1917, with MUSE r-band contours overlaid in white. Right panel: simulated PSF for the observation. We find no evidence for any extended emission superposed over the PSF. We do, however, make note of a semicircular arc of ∼10 excess counts ∼2″ SW of the nucleus and shown more clearly in Fig. A.4.
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.