Updated predictions for gravitational wave emission from tidal disruption events for next-generation observatories

Open Access

Fig. B.1.

Left panel: detection rates of WD-fTDEs from GCs plotted for different S/N thresholds. Right panel: GWB from WD-fTDEs from GCs. The color scheme and the detectors are the same as in Fig. 4-5. The solid line represents an intermediate-mass BH of 10³M_⊙, while the dotted line one of 500M_⊙.

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