Large late-type spiral galaxies in dense nearby filaments sit in patches where the Planck CMB is colder than in any of 10,000 simulations, at 5.7 sigma.
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A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter
Large late-type spiral galaxies in dense nearby filaments sit in patches where the Planck CMB is colder than in any of 10,000 simulations, at 5.7 sigma.