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

38 papers

astro-ph.CO2023★ 12 cited

Galaxy cluster mass accretion rates from IllustrisTNG

Michele Pizzardo, Margaret J. Geller, Scott J. Kenyon +2

We use simulated cluster member galaxies from Illustris TNG300-1 to develop a technique for measuring the galaxy cluster mass accretion rate (MAR) that can be applied directly to o…

astro-ph.CO2023★ 11 cited

An IllustrisTNG View of the Caustic Technique for Galaxy Cluster Mass Estimation

Michele Pizzardo, Margaret J. Geller, Scott J. Kenyon +2

The TNG300-1 run of the IllustrisTNG simulations includes 1697 clusters of galaxies with M covering the redshift range . We build mock spectros…

astro-ph.IM2023★ 28 cited

Identification of tidal features in deep optical galaxy images with Convolutional Neural Networks

H. Domínguez Sánchez, G. Martin, I. Damjanov +14

Interactions between galaxies leave distinguishable imprints in the form of tidal features which hold important clues about their mass assembly. Unfortunately, these structures are…

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.CO2022★ 15 cited

HectoMAP: The Complete Redshift Survey (Data Release 2)

Jubee Sohn, Margaret J. Geller, Ho Seong Hwang +3

HectoMAP is a dense redshift survey of 95,403 galaxies based primarily on MMT spectroscopy with a median redshift . The survey covers 54.64 square degrees in a 1.5$^\cir…

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…