MOIRCS Deep Survey V: A Universal Relation for Stellar Mass and Surface Brightness of Galaxies
Takashi Ichikawa, Masaru Kajisawa, Toru Yamada, Masayuki Akiyama,, Tomohiro Yoshikawa, Masato Onodera, Masahiro Konishi

TL;DR
This study reveals a universal linear relation between stellar mass and surface brightness in galaxies across redshifts 0.3 to 3, indicating similar mass assembly processes regardless of galaxy mass.
Contribution
It identifies a redshift-independent slope in the stellar mass–surface brightness relation and demonstrates that galaxy evolution is consistent with pure luminosity evolution up to z~3.
Findings
Universal linear correlation between stellar mass and surface brightness.
Surface brightness evolution follows (1+z)^(-2.0~-0.8).
Galaxy evolution aligns with pure luminosity evolution models.
Abstract
We present a universal linear correlation between the stellar mass and surface brightness (SB) of galaxies at 0.3<z<3, using a deep K-band selected catalog in the GOODS-North region. The correlation has a nearly constant slope, independent of redshift and color of galaxies in the rest-z frame. Considering unresolved compact galaxies, the tight correlation gives a lower boundary of SB for a given stellar mass; lower SB galaxies are prohibited over the boundary. The universal slope suggests that the stellar mass in galaxies was build up over their cosmic histories in a similar manner irrelevant to galaxy mass, as oppose to the scenario that massive galaxies mainly accumulated their stellar mass by major merging. In contrast, SB shows a strong dependence on redshift for a given stellar mass. It evolves as (1+z)^(-2.0~-0.8), in addition to dimming as (1+z)^4 by the cosmological expansion…
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