RECENTLY DESCRIBED. “As soon as the first submm galaxies were detected in 1997, it was clear that they made a significant contribution to the luminosity density in the high-redshift Universe, subject to the plausible assumptions that their SEDs were similar to those of luminous low-redshift dusty galaxies, and that their redshifts were not typically less than about z = 0.5.” (SED = spectral energy distribution).
https://lnkd.in/dAkZ_ejH
linkedin post 2022-06-29 05:12:48
Nigel Fleming
September 21, 2022