Table 5
Results of β-model fits to the radial distribution of FIRST sources associated with maxBCG clusters of galaxies, with the radio sources binned by luminosity L.
| Luminosity range | ζ | σ |
|
|
||
| log (L [W/Hz] ) < 23.8 | 0.0116 ± 0.0018 | 0.00249 ± 0.00067 |
| 23.8 ≤ log (L [W/Hz] ) < 24.2 | 0.0138 ± 0.0023 | 0.00319 ± 0.00054 |
| 24.2 ≤ log (L [W/Hz] ) < 24.6 | 0.0138 ± 0.0024 | 0.00343 ± 0.00073 |
| log (L [W/Hz] ) ≥ 24.6 | 0.0097 ± 0.0018 | 0.00303 ± 0.00088 |
Notes. Only the parameters ζ and σ, pertaining to the width of the profiles, are listed. β has been fixed to the best-fit value 0.987 from the total fit. The data are fitted using Eq. (4).
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