Strong detection of the CMB lensing and galaxy weak lensing cross ...
The amount of evolution in the dust content of galaxies over the past 5 billion years of cosmic history is contested in the literature.
DR6 Power Spectra, Likelihoods and ?CDM ParametersThe Pierre Auger Cosmic Ray Observatory. The Pierre Auger Collaborationa A. Aab, P. Abreu, M. Aglietta, E.J. Ahn, I.Al Samarai, J.N.. The far-infrared/radio correlation as probed by Herschel*The spectra are well fitted by a combination of free-free radiation, cosmic microwave background, thermal dust, and electric dipole radiation from small ... The Pierre Auger Cosmic Ray Observatory - HAL in2p3Aims. High-redshift dusty star-forming galaxies (DSFGs) are proposed to be the progenitors of massive quiescent galaxies arising at cosmic noon,.
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