Table 2.
GN-z11 physical parameters from BEAGLE SED fitting of the prism spectrum.
| Parameter | GN-z11 |
|---|---|
| log10(M/M⊙) |
 |
| ψ/M⊙ yr−1 |
 |
| log10(t/yr) |
 |
| log10(tM/yr) |
 |
| log10(Zneb/Z⊙) |
 |
| log10US |
 |
| AV |
 |
| log10(ξion/erg−1Hz) |
 |
| fesc |
 |
Notes. BEAGLE SED fitting of the prism spectrum of Fig. 2 with the uncertainties giving the extent of the 1σ credible regions: stellar mass (M, accounting for mass returned to the ISM through stellar winds and supernova explosions), star formation rate (ψ), maximum age of the stars (t), the mass-weighted age of stars (tM), nebular metallicity (Zneb), ionisation parameter (log10US), V-band dust attenuation (AV), ionising photon production efficiency (ξion) and escape fraction of H-ionising photons (fesc; see Appendix A for details).
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.