Spectral-line galaxy number counts and line intensity maps should show a kinematic dipole whose amplitude is set by the solar velocity and the frequency slope of the monopole, providing redundant multi-redshift measurements.
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Kinematically induced dipole anisotropy in line-emitting galaxy number counts and line intensity maps
Spectral-line galaxy number counts and line intensity maps should show a kinematic dipole whose amplitude is set by the solar velocity and the frequency slope of the monopole, providing redundant multi-redshift measurements.