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Gravitational-wave astronomers often wish to characterize the expected parameter-estimation accuracy of future observations.
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Inside the determinant, the first d d terms of the form C i j m [ N m − ( Δ h , \mathaccentV h a t 05 E n m ) ] C_{ij}^{m}[N_{m}-(\Delta h,\mathaccentV{hat}05E{n}_{m})] vanish because of the δ \delta s applied previously
Cited in the paper.
Formally, we see that Eq. ( 8
Cited in the paper.