Table E.2.
Best-fit parameters for the ṀSED-luminosity relation for each cluster derived by fitting Eq. (4) to the data.
| Cluster | Intercept (a) | Slope (b) | Intercept (a) |
|---|---|---|---|
| for fixed b = 4.8±0.6 | |||
| RSGC1 | −52.0±51.2 | 8.8±9.5 | −31.90±1.16 |
| NGC 2100 | −30.9±3.6 | 5.3±0.8 | −28.59±0.75 |
| NGC 7419 | −22.9±4.9 | 3.6±1.7 | −29.01±1.41 |
| χ Per | −27.06±4.90 | 4.5±1.0 | −28.97±0.99 |
Notes. The second and third column list, respectively, the intercept a and slope b with their standard deviation as derived by Beasor et al. (2020). The fourth column lists the intercept a and its standard deviation for a slope fixed to b = 4.8±0.6.
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.