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Fig. 4.
Phenomenological fits to the AT2017gfo light curve (with u dashed, q smooth and i dotted) shown in relation to the MeerLICHT 5σ limiting magnitudes. The shaded regions indicate the 1σ distance uncertainties. Apparent magnitudes were converted to absolute magnitudes using M = m − 5log10(dL/10 pc) at the distance of GW190814.
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