Figure 1

Distribution of the major axis of the sky position error ellipse, $2a$, for ${10}^4$ binaries with $m_1={10}^6{M}_{\odot }$ and $m_2=3\times {10}^5{M}_{\odot }$ at $z=1$. The dashed line is the precession-free calculation; the solid line includes precession. Sky position, as an extrinsic parameter, is improved somewhat indirectly by precession; therefore, the improvement is less than for the masses.Reuse & Permissions

Figure 2

Distribution of the minor axis of the sky position error ellipse, $2b$, for ${10}^4$ binaries with $m_1={10}^6{M}_{\odot }$ and $m_2=3\times {10}^5{M}_{\odot }$ at $z=1$. The dashed line is the precession-free calculation; the solid line includes precession.Reuse & Permissions

Figure 3

Distribution of errors in the luminosity distance for ${10}^4$ binaries with $m_1={10}^6{M}_{\odot }$ and $m_2=3\times {10}^5{M}_{\odot }$ at $z=1$. The dashed line is the precession-free calculation; the solid line includes precession.Reuse & Permissions