Image Details
Caption: Figure 9.
Effect of the warmer CMB on the recovered dust emission at 100 GHz as a function of redshift. We assume three different Tdust at z = 0, and plot the ratio between the intrinsic flux emitted by that galaxy at z = 0 and what can be recovered as the warmer CMB increases in temperature at higher redshift.
© 2025. The Author(s). Published by the American Astronomical Society.