Fig. 3.

Comparison of molecular gas mass (as traced via CO line emission), radio luminosity, and Lyα luminosity in ELANe, in high-redshift radio galaxies, and in z > 1 radio loud quasars (see Sect. 4 for references). For the Spiderweb, MAMMOTH-I, Slug, and Jackpot systems, we show (i) the total molecular gas mass of the system (circles), (ii) the molecular gas mass of the radio-loud AGN, if any (squares), and (iii) the molecular gas mass of the source considered to be the main powering source of the ELAN (triangles). The apparent correlation between molecular gas and radio luminosity appears to reflect selection effects. No clear correlation is found between the Lyα luminosity and other quantities. The lack of clear scaling relations highlight the complexity and diversity of these systems and of the physical and radiative processes that are occurring.
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