Table 3.
Results of the SED modelling.
| Type SFH | [Z/H]full | log10(Age/yr) | log10(Mstar/M⊙) | log10(LHα, int/erg s−1) |  |
|---|---|---|---|---|---|
| Burst, bin, Chab100 |
 |
 |
 |
 |
3.00 |
| Continuous, bin, Chab100 |
 |
 |
 |
 |
3.17 |
Notes. The uncertainties correspond to the 1σ intervals that are estimated following the standard method described in e.g. Avni (1976) assuming that the likelihood scales with 
The 
computed over the full MUSE spectrum of the best-fit models are listed in the right-most column. The best-fit stellar attenuation is E
for the burst and continuous models.
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.