Fig. 6.
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MOA-2011-BLG-191/OGLE-2011-BLG-0462 unabsorbed predicted spectrum. The interaction structure, accretion, and total emission are shown in light blue, light red and dark red, respectively. The 3-σ upper limits from the TGSS, RACS and VLASS catalogues are shown with green, cyan and orange arrows, while the upper limits from Mereghetti et al. (2022) are shown in magenta. The SKA and ngVLA sensitivity curves correspond to an integration time of 2 h (Sokolowski et al. 2022; McKinnon et al. 2019).
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