Table 1: Best fit values of the parameters of the evolutionary models for canonical radio sources.
Source type Luminosity function Evolution

$\log n_0~(\hbox{Mpc}^{-3})$ a b $\log L_\ast~(\hbox{erg}~\hbox{s}^{-1}~\hbox{Hz}^{-1}@5~\hbox{GHz},z=0)$ $k_{\rm ev}$ $z_{\rm top}$

FSRQ -8.988 0.651 2.888 34.043 0.224 2.252

BL Lac -7.921 0.977 1.266 32.789 0.745

Steep -8.030 1.071 3.054 33.329 4.902

**Table 1:** Best fit values of the parameters of the evolutionary models for canonical radio sources.
Source type	Luminosity function		Evolution
	$\log n_0~(\hbox{Mpc}^{-3})$	a	b	$\log L_\ast~(\hbox{erg}~\hbox{s}^{-1}~\hbox{Hz}^{-1}@5~\hbox{GHz},z=0)$	$k_{\rm ev}$	$z_{\rm top}$
FSRQ	-8.988	0.651	2.888	34.043	0.224	2.252
BL Lac	-7.921	0.977	1.266	32.789	0.745
Steep	-8.030	1.071	3.054	33.329	4.902

Source LaTeX | All tables | In the text

	1 Introduction
	2 The evolutionary model for canonical radio source populations
	3 Data sets
	4 Special source populations
	5 Sunyaev-Zeldovich effects
	6 Discussion and conclusions
	References