79 citations · 96 across the 5 of their papers we have counts for
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Cluster vs Field: Clear Evidence for a Morphology-Density Relation in All Environments at
Westley Brown, Adam Muzzin, Jasleen Matharu +6
We explore the relationship between galaxy structure, stellar mass, and local galaxy density in three SpARCS clusters at and compare with field galaxies from the 3D-HST…
CANUCS/Technicolor Data Release 2: A Catalogue of Galaxy Structural Parameters in up to 29 HST+JWST bands and a Multi-Wavelength Exploration of the Galaxy Size-Mass Relation at
Maya Merchant, Lamiya A. Mowla, Georgios E. Magdis +23
We present James Webb Space Telescope (JWST) results of a morphological study of galaxies in the CAnadian NIRISS Unbiased Cluster (CANUCS) and Technicolor surveys, observed in 19 m…
Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency
Lawrence Faria, David R. Patton, Stéphane Courteau +2
Using the TNG100-1 cosmological simulations, we explore how galaxy properties, such as specific star formation rate (), gas fraction ($\rm f_{gas} \,= \, M_{\rm H…
Interacting galaxies in the IllustrisTNG simulations -- V: Comparing the influence of star-forming vs. passive companions
Westley Brown, David R. Patton, Sara L. Ellison +1
We study interacting galaxy pairs in the TNG100-1 and TNG300-1 cosmological simulations using previously generated closest companion samples. We study the specific star formation r…
Interacting galaxies in the IllustrisTNG simulations -- I: Triggered star formation in a cosmological context
David R. Patton, Kieran D. Wilson, Colin J. Metrow +7
We use the IllustrisTNG cosmological hydrodynamical simulations to investigate how the specific star formation rates (sSFRs) of massive galaxies depend on…