Mollweide view of the sky showing the locations of all giants and LoTSS DR1 RGs in the Local Universe for which we inferred Cosmic Web densities and dynamical states. The background shows the Milky Way at 150 MHz (Zheng et al. 2017), on which we overlaid the LoTSS DR1 footprint (hatched dark rectangle). All RGs are drawn as lemniscates of Bernoulli; we did not attempt to portray realistic shapes or position angles. The colours represent redshifts z ∈ (0, z_max ≔ 0.16), whilst the diameters are proportional to projected proper lengths l_p ∈ ( ∼ 1 kpc, 4.6 Mpc). Giants are translucent. Upon zooming in, the reader can appreciate the wide variety of observed radio galaxy sizes.