Spatial distribution of CGs identified in GAMA equatorial fields (large filled dots). In this case, the sample of CGs is the CG-m2V5, i.e. with members within a two-magnitude gap and a maximum velocity separation from the CG centre of 500 km s⁻¹. Each cone displays the CG positions using the right ascension and redshift in each field. The colour distribution shows the r-band apparent magnitude of the brightest galaxy in the CG. The black points show a random sample of galaxies (∼20%) in the main survey.