activity
19992020
most citedAt the heart of the matter: the origin of bulgeless dwarf galaxies and Dark Matter cores

1k citations · 5.8k across the 37 of their papers we have counts for

collaborators

37 papers

astro-ph.IM2020★ 3 cited

Supernova Model Discrimination with Hyper-Kamiokande

Jost Migenda

Supernovae are among the most magnificent events in the observable universe. They produce many of the chemical elements necessary for life to exist and their remnants---neutron sta…

astro-ph.CO2013★ 19 cited

The Spatial Extent and Distribution of Star Formation in 3D-HST Mergers at z~1.5

Kasper B. Schmidt, Hans-Walter Rix, Elisabete da Cunha +14

We present an analysis of the spatial distribution of star formation in a sample of 60 visually identified galaxy merger candidates at z>1. Our sample, drawn from the 3D-HST survey…

astro-ph.CO2013★ 61 cited

Global Star Formation Rates and Dust Emission Over the Galaxy Interaction Sequence

Lauranne Lanz, Andreas Zezas, Nicola Brassington +7

We measured and modeled the spectral energy distributions (SEDs) in 28 bands from the ultraviolet to the far-infrared (FIR) for 31 interacting galaxies in 14 systems. The sample is…

astro-ph.CO2012★ 207 cited

Submillimetre galaxies in a hierarchical universe: number counts, redshift distribution, and implications for the IMF

Christopher C. Hayward, Desika Narayanan, Dušan Kereš +4

High-redshift submillimetre galaxies (SMGs) are some of the most rapidly star-forming galaxies in the Universe. Historically, galaxy formation models have had difficulty explaining…

astro-ph.CO2012★ 48 cited

Modeling Mid-Infrared Diagnostics of Obscured Quasars and Starbursts

Gregory F. Snyder, Christopher C. Hayward, Anna Sajina +5

We analyze the link between active galactic nuclei (AGN) and mid-infrared flux using dust radiative transfer calculations of starbursts realized in hydrodynamical simulations. Focu…

astro-ph.GA2012★ 11 cited

On Galaxies and Homology

Gregory S. Novak, Patrik Jonsson, Joel R. Primack +2

The definition of homology for single-component galaxies is clear, but for multi-component (luminous and dark matter) galaxies there is some ambiguity. We attempt to clarify the si…