7 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…
Impact of stochastic star-formation histories and dust on selecting quiescent galaxies with JWST photometry
K. Lisiecki, D. Donevski, A. W. S. Man +16
While the James Webb Space Telescope (JWST) now allows identifying quiescent galaxies (QGs) out to early epochs, the photometric selection of quiescent galaxy candidates (QGCs) and…
Structural evolution of quiescent galaxies at intermediate redshifts at UV and red rest-frame wavelengths
Michele Pizzardo, Ivana Damjanov, Jubee Sohn +1
We model the wavelength dependence of structural parameters for a mass-limited sample () of quiescent galaxies with using $griz…
ALMA reveals diverse dust-to-gas mass ratios and quenching modes in old quiescent galaxies
Giuliano Lorenzon, Darko Donevski, Allison W. S. Man +18
Recent discoveries of dust and molecular gas in quiescent galaxies (QGs) up to challenge the long-standing view that the interstellar medium depletes rapidly once star for…
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…