Table 7:
Spectral data for 0222+36.
Frequency |
Total |
Halo |
Lobes |
Core |
(GHz) |
(mJy) |
(mJy) |
(mJy) |
(mJy) |
0.074 (VLSS) |
580 |
- |
- |
- |
0.325 (WENSS) |
380 |
188a |
191b |
0.9b |
0.365 (TEXAS) |
352 |
174a |
177b |
1.2b |
0.408 (B2) |
337 |
170a |
165b |
1.8b |
1.4 (VLA) |
190 |
36 |
52 |
102
 |
5.0 (VLA) |
224 |
8 |
36 |
180 |
8.4 (VLA) |
192 |
nd |
26 |
166 |
22.5 (VLA) |
96 |
nd |
6 |
90 |
Notes - a The flux density of the halo is computed from subtraction of the
nuclear and lobe components from the total flux density listed in Col. 2; blobes and core flux densities at low frequency (0.325, 0.365, and 0.408 GHz)
are extrapolated from data between 1.4 and 22 GHz (see text); c from VLBA
data at 1.6 GHz.
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