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Fig. 5.

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LoTSS DR2 cutouts at central observing frequency νobs = 144 MHz and resolution θFWHM = 6″, centred around the hosts of newly discovered giants. Each cutout covers a solid angle of 6′×6′. Contours signify 3, 5, and 10 sigma-clipped standard deviations above the sigma-clipped median. For scale, we show the stellar Milky Way disk (with a diameter of 50 kpc) generated using the Ringermacher & Mead (2009) formula, alongside a 3 times inflated version. Each DESI Legacy Imaging Surveys DR9 (g, r, z) inset shows the central 1′×1′ square region. As all giants obey ϕ ≥ 1.3′, they must – if not oriented along one of the square’s diagonals – necessarily protrude from this region. Rowwise from left to right, from top to bottom, these giants are ILTJ002943.72+295700.3, ILTJ003010.58+170948.6, ILTJ003521.87+233625.9, ILTJ003712.91+284436.8, ILTJ004002.30+252550.9, and ILTJ235802.49+331838.5.

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