4 papers
Size-Mass Relation Shows Its Colours: Contrasting Physical Imprints of Galaxy Evolution in Rest-Frame UV and Optical
Angelo George, Marcin Sawicki, Ivana Damjanov
The galaxy size-mass relation (SMR) is a key scaling relation used to constrain the physical processes that build galaxy structure, yet it is almost always measured in a single res…
The Role of Cluster Environments in Quiescent Galaxy Stellar Halo Assembly
Devin J. Williams, Ivana Damjanov, Marcin Sawicki +6
External interactions drive galaxy stellar mass growth and morphological evolution. As stellar haloes-assembled largely via hierarchical accretion-preserve signatures of these proc…
Effects of Environment on the Size Evolution of Quiescent Galaxies: Comparing Galaxies in Clusters and in the Field at Two Rest-frame Wavelengths
Angelo George, Ivana Damjanov, Marcin Sawicki +9
We investigate the impact of environment on quiescent galaxy (QG) size evolution using the CLAUDS+HSC imaging covering 18.6~deg in five broad filters () and the effectiv…
The Growth of Galaxy Stellar Haloes Over
Devin J. Williams, Ivana Damjanov, Marcin Sawicki +9
Galaxies are predicted to assemble their stellar haloes through the accretion of stellar material from interactions with their cosmic environment. Observations that trace stellar h…