“The MeerKAT Absorption Line Survey Data Release 2: Wideband continuum catalogues and a measurement of the cosmic radio dipole” https://arxiv.org/abs/2408.16619
The assumption of isotropy in the number counts of radio sources seems to work on Gpc scales?
I have only read the abstract but it seems to say that their finding is consistent with the CMB dipole, meaning that the number count is NOT isotropic and over and underdensities follow the famous dipole shape.
They say after that they correct this systematic, the “declination effect” and yet they still find a dipole signal. I don’t understand the consequence of correcting for their systematic.
The ‘dipole shape’ is not considered an anisotropy but a result of our motion relative to the “CMB rest-frame”.
The systematic effect biases the data away from the result they want. After correcting for that systematic effect, the smaller dipole signal appears with the same amplitude as measured with the CMB. Since the CMB is isotropic (after removing contributions from multipoles) their conclusion is that the assumption of isotropy is correct.
I’m not saying I agree with their logic…
Figures 11 and 12 don’t seem to corroborate their “recovering the CMB dipole”.
The direction of the dipole is not that close
The amplitude of the dipole is not that close either
The Secrest et al. (2022) paper is the best of the lot so far in my opinion.