Free Access

Fig. 8


Spectral region around the Paschen limit. The red spectrum was extracted from the MUSE cube at the approximate position of slit1 of Baldwin et al. (1991). In gray, a typical Paranal sky spectrum is shown. Broad second-order contamination by prominent blue Balmer emission lines is marked in black.

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.