Table 5.
Observed B − V colour excess derived from Balmer decrement, as well as the integrated Hα flux and resulting SFR corrected for dust reddening and gravitational magnification.
| Component | E(B − V)BD | FHα, intrinsic | SFRHα |
|---|---|---|---|
| C | 0.58 ± 0.14 | 4.6 ± 2.3 | 160 ± 80 |
| S1 | 0.22 ± 0.05 | 1.6 ± 0.3 | 58 ± 10 |
| S2 | 0.18 ± 0.09 | 0.8 ± 0.2 | 29 ± 9 |
| W1 | 0.27 ± 0.16 | 2.8 ± 1.6 | 100 ± 60 |
| W2 | 0.52 ± 0.17 | 4.4 ± 2.8 | 160 ± 100 |
Notes. Flux and SFR values are in units of [10−17 erg s−1 cm−2] and [M⊙ yr−1], respectively. We assume a Salpeter (1955) IMF and Calzetti et al. (2000) extinction law.
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.