37 citations · 62 across the 12 of their papers we have counts for
12 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…
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…
The average stellar population age and metallicity of intermediate-redshift quiescent galaxies
Ivana Damjanov, Margaret J. Geller, Jubee Sohn
The HectoMAP spectroscopic survey provides a unique mass-limited sample of more than 35,000 quiescent galaxies () covering the redshift range . We segregate…
Two rest-frame wavelength measurements of galaxy sizes at : the evolutionary effects of emerging bulges and quenched newcomers
Angelo George, Ivana Damjanov, Marcin Sawicki +6
We analyze the size evolution of star-forming galaxies (SFGs) and quiescent galaxies (QGs) with mass at from the COSMOS field using…
The splashback radius and the radial velocity profile of galaxy clusters in IllustrisTNG
Michele Pizzardo, Margaret J. Geller, Scott J. Kenyon +1
We use 1697 clusters of galaxies from the Illustris TNG300-1 simulation (mass M and redshift range ) to explore the physics of the c…
In pursuit of giants: II. Evolution of dusty quiescent galaxies over the last six billion years from the hCOSMOS survey
Darko Donevski, Ivana Damjanov, Ambra Nanni +11
Quantifying changes in galaxies' interstellar medium (ISM) abundance after quenching star formation is an important aspect of galaxy evolution, but it is poorly constrained beyond…
Co-evolution of the Brightest Cluster Galaxies and their Host Clusters in IllustrisTNG
Jubee Sohn, Margaret J. Geller, Mark Vogelsberger +1
We use the IllustrisTNG simulations to explore the dynamic scaling relation between massive clusters and their central galaxies (BCGs). The Illustris TNG300-1 simulation we use inc…
Quiescent Galaxy Size and Spectroscopic Evolution: Combining HSC Imaging and Hectospec Spectroscopy
Ivana Damjanov, H. Jabran Zahid, Margaret J. Geller +3
We explore the relations between size, stellar mass and average stellar population age (indicated by D indices) for a sample of intermediate-redshift galaxies f…