http://arxiv.org/abs/2205.06880
An observer moving with respect to the cosmic rest frame should observe a concentration and brightening of galaxies in the direction of motion and a spreading and dimming in the opposite direction. The velocity inferred from this dipole should match that of the cosmic microwave background (CMB) temperature dipole if galaxies are on average at rest with respect to the CMB rest frame. However, recent studies have claimed a many-fold enhancement of galaxy counts and flux in the direction of the solar motion compared to the CMB expectation, calling into question the standard cosmology. Here we show that the sky distribution and brightness of extragalactic radio sources are consistent with the CMB dipole in direction and velocity. We use the first epoch of the Very Large Array Sky Survey combined with the Rapid Australian Square Kilometer Array Pathfinder Continuum Survey to estimate the dipole via several different methods, and all show similar results. Typical fits find a $331^{+161}{-107}$ km s$^{-1}$ velocity dipole with apex $(\ell,b) = (271^{+55}{-58}, 56^{+13}{-35})$ in Galactic coordinates from source counts and $399^{+264}{-199}$ km s$^{-1}$ toward $(\ell,b) = (301^{+30}{-30}, 43^{+19}{-17})$ from radio fluxes. These are consistent with the CMB-solar velocity, 370 km s$^{-1}$ toward $(\ell,b) = (264, 48)$, and show that galaxies are on average at rest with respect to the rest frame of the early universe, as predicted by the canonical cosmology.
J. Darling
Tue, 17 May 22
1/95
Comments: 11 pages, 5 figures, 1 table. Accepted by ApJL