Open Access
). We assume optimal orientation of detector and source as well as the GW to be emitted along the polar axis.


Table 2:


$\Omega _{c,i}$ [rad s-1] Overlap
R1E1ACL 0.3 96%
R3E1ACL 2$\pi$ 92%
R4E1ACL 3$\pi$ 97%

Source LaTeX | All tables | In the text

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