Free Access

Fig. 5.

image

Completeness as a function of magnitude for all MUSE observations of NGC 3201, using photometry from the ACS globular cluster survey (Sarajedini et al. 2007). The fraction of all possible extracted spectra to observed spectra within the MUSE FoV is shown. Blue: extracted spectra with S/N >  2. Orange: extracted spectra in the final sample (see Sect. 3.2). (The uncertainties are smaller than the points.)

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.