Kinematic dipole detection with galaxy surveys: forecasts and
  requirements
  Upcoming or future deep galaxy samples with wide sky coverage can provide
independent measurement of the kinematic dipole - our motion relative to the
rest frame defined by the large-scale structure. Such a measurement would
present an important test of the standard cosmological model, as the standard
model predicts the galaxy measurement should precisely agree with the existing
precise measurements made using the CMB. However, the required statistical
precision to measure the kinematic dipole typically makes the measurement
susceptible to bias from the presence of the local-structure-induced dipole
contamination. In order to minimize the latter, a sufficiently deep survey is
required. We forecast both the statistical error and the systematic bias in the
kinematic dipole measurements. We find that a survey covering $\sim 75\%$ of
the sky in both hemispheres and having $\sim 30$ million galaxies can detect
the kinematic dipole at $5\sigma$, while its median redshift should be at least
$z_{med} \sim 0.75$ for negligible bias from the local structure.
