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.
|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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