activity
20062023
most citedRed Nuggets at z~1.5: Compact passive galaxies and the formation of the Kormendy Relation

346 citations · 1.7k across the 38 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

25 papers · 1 filter

astro-ph.GA2022★ 11 cited

Size and Spectroscopic Evolution of HectoMAP Quiescent Galaxies

Ivana Damjanov, Jubee Sohn, Margaret J. Geller +2

The HectoMAP survey provides a complete, mass-limited sample of 30,231 quiescent galaxies with band Hyper Suprime-Cam Subaru Strategic Program (HSC SSP) imaging that spans the…

astro-ph.GA2022★ 12 cited

Stellar Masses of Clumps in Gas-rich, Turbulent Disk Galaxies

Liyualem Ambachew, Deanne B. Fisher, Karl Glazebrook +6

In this paper we use HST/WFC3 observations of 6 galaxies from the DYNAMO survey, combined with stellar population modelling of the SED, to determine the stellar masses of DYNAMO cl…

astro-ph.GA2021

Quiescent Galaxy Size, Velocity Dispersion, and Dynamical Mass Evolution

Ivana Damjanov, Jubee Sohn, Yousuke Utsumi +2

We use surveys covering the redshift range to explore quiescent galaxy scaling relations and the redshift evolution of the velocity dispersion, size, and dynamical…

astro-ph.GA2021★ 87 cited

Hyper Suprime-Cam Subaru Strategic Program: A Mass-Dependent Slope of the Galaxy Size-Mass Relation at

Lalitwadee Kawinwanichakij, John D. Silverman, Xuheng Ding +11

We present the galaxy size-mass () distributions using a stellar-mass complete sample of million galaxies, covering deg, with $\log(M_{\ast}…

astro-ph.GA2020★ 16 cited

CANDELS Meets GSWLC: Evolution of the Relationship Between Morphology and Star Formation Since z = 2

Chandler Osborne, Samir Salim, Ivana Damjanov +7

Galaxy morphology and its evolution over the cosmic epoch hold important clues for understanding the regulation of star formation (SF). However, studying the relationship between m…

astro-ph.GA2019

Size-scaling of clump instabilities in turbulent, feedback regulated disks

Kamran Ali, Danail Obreschkow, Liang Wang +5

We explore the scaling between the size of star-forming clumps and rotational support in massively star-forming galactic disks. The analysis relies on simulations of a clumpy galax…