Free Access
Table 3.
Peak energy densities of the radiation fields for all 16 of our sample of star-forming galaxies during their starburst phase, compared to the energy density of the CMB radiation field at their observed redshift.
| Galaxy ID | U*/eV cm−3 | UCMB/eV cm−3 |
|---|---|---|
| HDFN-3654-1216 | 50 | 800 |
| UDF-640-1417 | 110 | 1000 |
| GNS-zD2 | 92 | 1200 |
| CDFS-3225-4627 | 120 | 1200 |
| GNS-zD4 | 200 | 1200 |
| GNS-zD1 | 370 | 1200 |
| GN-108036 | 380 | 1200 |
| SXDF-NB1006-2 | 530 | 1200 |
| UDF-983-964 | 36 | 1300 |
| GNS-zD3 | 150 | 1300 |
| GNS-zD5 | 370 | 1300 |
| A1689-zD1 | 11 | 1500 |
| EGS-zs8-1 | 190 | 1600 |
| UDF-3244-4727 | 160 | 1700 |
| MACS1149-JD1 | 6.6 | 2800 |
| GN-z11 | 630 | 5800 |
Notes. This shows that, in all cases, radiative cooling of the CR electrons would be dominated by the CMB.
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.