Fig. 1.
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GW signal from a fTDE of a 0.1 M⊙ MS star disrupted by a 4 × 106 M⊙ BH (gray lines) and GW signal from a fTDE of a WD of 0.5 M⊙ disrupted by a 103 M⊙ BH (red lines). We consider two possible source distances: 8 kpc (dashed lines) and 1 Mpc (dash-dotted lines). In blue and orange, we plot the noise amplitudes of LISA and DO, respectively.
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