pinball1970
Gold Member
2025 Award
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- TL;DR
- Massive early-type galaxies contribute a non-negligible source of CMB foreground contamination. Even in our most conservative estimates, massive ETGs account for 1.4% up to the full present-day CMB energy density.
The impact of early massive galaxy formation on the cosmic microwave background
The paper here.https://www.sciencedirect.com/science/article/pii/S0550321325001403?via=ihub
From the conclusions
"What results from these estimates, naturally but unexpectedly, is as follows. Under the most conservative assumptions – i.e., assuming that the average ETG separation {D0 (nought)} in local volumes applies to the whole Universe – the formation of massive ETGs may account for 1.4% of the observed (present-day) CMB photon energy density. If, instead, (D0) corresponds to that inferred around Z~2 [32], then the cumulative energy density of massive ETGs would be of the same order as that of the observed CMB (Fig. 5). Assuming that dust produced by massive ETGs reaches thermal equilibrium with the ETG radiation field, the resulting emission would form a background near Z~15 that, when redshifted, appears to observers at Z=0 as a microwave photon field (Sec. 3.2). The independent data now coming from the observations with the JWST of the formation of massive galaxies at Z>9 and the ALMA observations of high-redshift, dust-rich, star-forming galaxies support this conclusion, as do the recent observationally obtained mass-growth times and rates of individual elliptical galaxies (Fig. 3)."

