Table 2
Radio morphological classification and some properties of the polarized radio galaxies in the ELAIS-N1 LOFAR Deep Field.
| Type | N | Fraction | ID of polarized component in Paper I |
|---|---|---|---|
| Compact | 4 | 12.9 ± 6.5% | 09, 10, 24, 25 |
| FRI | 4 | 12.9 ± 6.5% | 06, 14, 18, 32 |
| FRII | 18 | 58.1 ± 13.7% | 01, 02, 04A + 04B; 05, 07, 08, 11, 12; 13A(a) +29; 15, 17, 19, 21, 23, 26, 27(b), 30, 31(b) |
| Other Extended | 5 | 16.1 ± 7.2% | 03, 16, 20(c), 22, 28 |
| Total | 31 | 100% | |
| Radio size > 500 kpc | 9 | 29.0 ± 9.7% | 08, 11, 12; 13A + 29; 15, 18, 23, 26, 32 |
| Radio size > 1 Mpc | 3 | 9.7 ± 5.6% | 11, 12, 23 |
Notes. N is the number of radio galaxies. The uncertainties associated with the fractional number of sources of a given type are Poissonian (
). a) Sources 13A and 29 (13B) are two lobes of the same FRII radio galaxy. b) Source 27 and 31 were classified as FRIs by Mingo et al. (2022), but after visual inspection, we classified them as FRIIs. c) Source 20 appears to be a one-sided blazar.
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.