Cookie-cutter halos: the remarkable constancy of the stellar mass function of satellite galaxies at 0.2<z<1.2
Tomer Tal, Ryan F. Quadri, Adam Muzzin, Danilo Marchesini, Mauro, Stefanon

TL;DR
This study reveals that the stellar mass function of satellite galaxies remains remarkably consistent across redshifts 0.2 to 1.2 and varies primarily with the mass of the central galaxy, indicating a universal pattern in galaxy group evolution.
Contribution
It demonstrates the near-universality of satellite galaxy mass functions across redshifts and links satellite growth to central galaxy mass, using statistical background subtraction techniques.
Findings
Satellite stellar mass functions increase with central galaxy mass.
Minimal redshift dependence of satellite mass functions at fixed central mass.
Quiescent satellite fraction increases with central galaxy mass.
Abstract
We present an observational study of the stellar mass function of satellite galaxies around central galaxies at 0.2<z<1.2. Using statistical background subtraction of contaminating sources we derive satellite stellar mass distributions in four bins of central galaxy mass in three redshift ranges. Our results show that the stellar mass function of satellite galaxies increases with central galaxy mass, and that the distribution of satellite masses at fixed central mass is at most weakly dependent on redshift. We conclude that the average mass distribution of galaxies in groups is remarkably universal even out to z=1.2 and that it can be uniquely characterized by the group central galaxy mass. This further suggests that as central galaxies grow in stellar mass, they do so in tandem with the mass growth of their satellites. Finally, we classify all galaxies as either star forming or…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Scientific Research and Discoveries
