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Fig. 3.
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Absolute flux obtained at t = 0.5, 1, 5 days after the merger as seen by MAAT using R1000B and R1000R gratings. We plot run 1 (EoS DD2) for a polar and equatorial observer (dark and pale blue lines). Same for run 7 (EoS LS220) for a polar and equatorial observer (red and orange lines). A distance of 40 Mpc is assumed.
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