Fig. 4
Optical to X-ray SED for Mrk 1018 for two epochs. Shown are the photometry of the nucleus in the SDSS r and u band (see Paper I), the NUV and FUV from GALEX and HST observations, and the unabsorbed power-law X-ray spectrum from Chandra. The black dashed line represents a model for a geometrically thin relativistic accretion disc as described in the text.
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.