Table 3
Radio size, radio power and kinetic jet energy estimates.
Source | LAS | LAS | log P500 | log P1.4 | log P151 | log Emech,W | log Emech,C | |
[arcsec] | [kpc] | [W Hz-1] | [W Hz-1] | [W Hz-1] | [erg s-1] | [erg s-1] | ||
|
||||||||
MRC 0114-211 | 0.7 | 5.9 | 28.8 ± 0.1 | 28.6 ± 0.1 | 29.1 ± 0.1 | 47.0 ± 0.3 | 47.4 ± 0.3 | |
TN J0121+1320 | 0.3 | 2.2 | 28.5 ± 0.1 | 28.0 ± 0.1 | 29.1 ± 0.1 | 47.0 ± 0.3 | 47.0 ± 0.3 | |
BRL 0128-264 | 35.8 | 293.6 | 29.1 ± 0.1 | 28.8 ± 0.1 | 29.7 ± 0.1 | 47.5 ± 0.3 | 46.6 ± 0.3 | |
MRC 0156-252 | 8.3 | 69.7 | 28.5 ± 0.1 | 28.0 ± 0.1 | 28.9 ± 0.1 | 46.8 ± 0.3 | 47.0 ± 0.3 | |
TN J0205+2242 | 2.7 | 19.7 | 28.5 ± 0.1 | 28.0 ± 0.1 | 29.1 ± 0.1 | 47.0 ± 0.3 | 47.0 ± 0.3 | |
USS 0211-122 | 16.2 | 132.8 | 28.5 ± 0.1 | 28.0 ± 0.1 | 29.0 ± 0.1 | 46.9 ± 0.3 | 47.0 ± 0.3 | |
MRC 0251-273 | 0.9 | 6.8 | 28.5 ± 0.1 | 28.3 ± 0.1 | 29.0 ± 0.1 | 46.9 ± 0.3 | 47.2 ± 0.3 | |
RC J0311+0507 | 2.8 | 18.5 | 29.5 ± 0.1 | 29.1 ± 0.1 | 30.0 ± 0.1 | 47.7 ± 0.3 | 47.8 ± 0.3 | |
MRC 0316-257 | 7.6 | 57.8 | 29.0 ± 0.1 | 28.5 ± 0.1 | 29.5 ± 0.1 | 47.3 ± 0.3 | 47.4 ± 0.3 | |
MP J0340-6507 | 20.0 | 164.0 | 28.8 ± 0.1 | 28.3 ± 0.1 | 29.5 ± 0.1 | 47.3 ± 0.3 | 47.2 ± 0.3 | |
MRC 0406-244 | 7.3 | 59.1 | 29.0 ± 0.1 | 28.6 ± 0.1 | 29.7 ± 0.1 | 47.5 ± 0.3 | 47.5 ± 0.3 | |
PKS 0529-549 | 1.0 | 8.0 | 29.2 ± 0.1 | 28.6 ± 0.1 | 29.8 ± 0.1 | 47.6 ± 0.3 | 47.5 ± 0.3 | |
TXS 0828+193 | 20.0 | 160. | 28.4 ± 0.1 | 27.9 ± 0.1 | 29.0 ± 0.1 | 46.9 ± 0.3 | 46.9 ± 0.3 | |
5C 7.269 | 0.5 | 4.2 | 27.8 ± 0.1 | 27.4 ± 0.1 | 28.3 ± 0.1 | 46.3 ± 0.3 | 46.6 ± 0.3 | |
MRC 1017-220 | 8.3 | 70.6 | 28.1 ± 0.1 | 27.9 ± 0.1 | 28.2 ± 0.1 | 46.2 ± 0.3 | 46.9 ± 0.3 | |
TN J1112-2948 | 3.1 | 23.6 | 28.8 ± 0.1 | 28.2 ± 0.1 | 29.5 ± 0.1 | 47.3 ± 0.3 | 47.2 ± 0.3 | |
TXS 1113-178 | 10.3 | 84.5 | 28.5 ± 0.1 | 28.1 ± 0.1 | 29.0 ± 0.1 | 46.9 ± 0.3 | 47.1 ± 0.3 | |
3C 257 | 12.8 | 103.7 | 29.2 ± 0.1 | 29.1 ± 0.1 | 29.4 ± 0.1 | 47.2 ± 0.3 | 47.8 ± 0.3 | |
MRC 1138-262 | 11.4 | 94.6 | 29.1 ± 0.1 | 28.6 ± 0.1 | 29.7 ± 0.1 | 47.5 ± 0.3 | 47.5 ± 0.3 | |
USS 1243+036 | 7.0 | 51.1 | 29.2 ± 0.1 | 28.7 ± 0.1 | 29.9 ± 0.1 | 47.7 ± 0.3 | 47.5 ± 0.3 | |
MG 1251+1104 | 1.2 | 9.8 | 28.4 ± 0.1 | 28.0 ± 0.1 | 28.9 ± 0.1 | 46.8 ± 0.3 | 47.0 ± 0.3 | |
MRC 1324-262 | 1.7 | 13.9 | 28.5 ± 0.1 | 28.1 ± 0.1 | 28.9 ± 0.1 | 46.8 ± 0.3 | 47.1 ± 0.3 | |
TN J1338-1942 | 1.4 | 9.7 | 28.7 ± 0.1 | 28.3 ± 0.1 | 29.3 ± 0.1 | 47.1 ± 0.3 | 47.2 ± 0.3 | |
USS 1410-001 | 23.5 | 192.7 | 28.4 ± 0.1 | 28.0 ± 0.1 | 29.0 ± 0.1 | 46.9 ± 0.3 | 47.0 ± 0.3 | |
MRC 1558-003 | 7.7 | 62.4 | 28.8 ± 0.1 | 28.4 ± 0.1 | 29.5 ± 0.1 | 47.3 ± 0.3 | 47.3 ± 0.3 | |
USS 1707+105 | 21.7 | 177.9 | 28.6 ± 0.1 | 28.2 ± 0.1 | 29.1 ± 0.1 | 47.0 ± 0.3 | 47.2 ± 0.3 | |
3C 362 | 6.9 | 56.6 | 28.9 ± 0.1 | 28.6 ± 0.1 | 29.4 ± 0.1 | 47.2 ± 0.3 | 47.5 ± 0.3 | |
MP 1758-6738 | 40 | 336. | 29.0 ± 0.1 | 28.0 ± 0.1 | 28.5 ± 0.1 | 47.3 ± 0.3 | 47.0 ± 0.3 | |
TN J2007-1316 | 12 | 85.2 | 29.1 ± 0.1 | 28.5 ± 0.1 | 29.9 ± 0.1 | 47.7 ± 0.3 | 47.4 ± 0.3 | |
MRC 2025-218 | 5.1 | 40.8 | 28.7 ± 0.1 | 28.3 ± 0.1 | 29.3 ± 0.1 | 47.1 ± 0.3 | 47.2 ± 0.3 | |
MG 2037-0011 | 0.2 | 1.7 | 27.9 ± 0.1 | 27.6 ± 0.1 | 28.2 ± 0.1 | 46.7 ± 0.3 | 46.2 ± 0.3 | |
MRC 2048-272 | 6.7 | 55.6 | 28.7 ± 0.1 | 28.2 ± 0.1 | 29.4 ± 0.1 | 47.2 ± 0.3 | 47.2 ± 0.3 | |
MRC 2104-242 | 21.8 | 176.6 | 28.8 ± 0.1 | 28.4 ± 0.1 | 29.5 ± 0.1 | 47.3 ± 0.3 | 47.3 ± 0.3 | |
4C 23.56 | 47.0 | 380.7 | 28.9 ± 0.1 | 28.4 ± 0.1 | 29.5 ± 0.1 | 47.3 ± 0.3 | 47.3 ± 0.3 | |
NVSS J2135−3337 | 0.5 | 4.1 | 27.0 ± 0.1 | 27.2 ± 0.1 | 28.5 ± 0.1 | 46.5 ± 0.3 | 46.4 ± 0.3 | |
MG 2144+1928 | 8.5 | 62.0 | 29.1 ± 0.1 | 28.6 ± 0.1 | 29.6 ± 0.1 | 47.4 ± 0.3 | 47.5 ± 0.3 | |
MRC 2224-273 | 0.4 | 3.3 | 27.8 ± 0.1 | 27.6 ± 0.1 | 27.9 ± 0.1 | 45.9 ± 0.3 | 46.7 ± 0.3 | |
TN J2254+1857 | 2.7 | 22.4 | 27.8 ± 0.1 | 27.2 ± 0.1 | 28.5 ± 0.1 | 46.5 ± 0.3 | 46.4 ± 0.3 | |
MG 2308+0336 | 3.6 | 29.2 | 28.5 ± 0.1 | 28.3 ± 0.1 | 28.9 ± 0.1 | 46.8 ± 0.3 | 47.2 ± 0.3 | |
TXS 2353-003 | 38.8 | 310.4 | 28.8 ± 0.1 | 28.3 ± 0.1 | 29.3 ± 0.1 | 47.1 ± 0.3 | 47.2 ± 0.3 |
Notes. Errors are the measurement uncertainties, except for the kinetic power where we use the scatter in the relationships we used to derive our estimates. We do not provide uncertainties for the Largest Angular Scale, because these are strongly dominated by the dynamic range, resolution, and frequency of the data set used, which in our case is rather heterogeneous. For all but the very compact sources, these uncertainties are in the range of few percent.
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