Papers

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2016 Iryna Butsky

, Liang Wang, Aura Obreja, Greg S. Stinson, Camilla Penzo, Xi Kang, Ben W. Keller, James Wadsley

NIHAO project II: halo shape, phase-space density and velocity distribution of dark matter in galaxy formation simulations

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Camilla Penzo, Andrea V. Macciò, Marco Baldi, Luciano Casarini, Jose Oñorbe, Aaron A. Dutton

Effects of coupled dark energy on the Milky Way and its satellites

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Tobias Buck

, Aaron A. Dutton

, Andrea V. Macciò

Simulated ΛCDM analogues of the thin plane of satellites around the Andromeda galaxy are not kinematically coherent structures

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Aura Obreja, Gregory S. Stinson, Aaron A. Dutton

, Andrea V. Macciò, Liang Wang, Xi Kang

NIHAO VI. The hidden discs of simulated galaxies

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Aaron A. Dutton

, Andrea V. Macciò, Jonas Frings, Liang Wang, Gregory S. Stinson, Camilla Penzo, Xi Kang

NIHAO V: too big does not fail – reconciling the conflict between ΛCDM predictions and the circular velocities of nearby field galaxies

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2015 Akın Yıldırım, Remco C. E. van den Bosch, Glenn van de Ven

, Aaron Dutton

, Ronald Läsker, Bernd Husemann, Jonelle L. Walsh, Karl Gebhardt, Kayhan Gültekin

, Ignacio Martín-Navarro

The massive dark halo of the compact early-type galaxy NGC 1281

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Liang Wang, Aaron A. Dutton

, Gregory S. Stinson, Andrea V. Macciò, Camilla Penzo, Xi Kang, Ben W. Keller, James Wadsley

NIHAO project – I. Reproducing the inefficiency of galaxy formation across cosmic time with a large sample of cosmological hydrodynamical simulations

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Stéphane Courteau

, Aaron A. Dutton

On the Global Mass Distribution in Disk Galaxies

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2014 X. C. Dong, W. P. Lin

, X. Kang, Yang Ocean Wang

, Aaron A. Dutton

, Andrea V. Macciò

The Distribution of Satellites Around Central Galaxies in a Cosmological Hydrodynamical Simulation

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Aaron A. Dutton

, Andrea V. Macciò

Cold dark matter haloes in the Planck era: evolution of structural parameters for Einasto and NFW profiles

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Arianna Di Cintio, Chris B. Brook, Aaron A. Dutton

, Andrea V. Macciò, Greg S. Stinson, Alexander Knebe

A mass-dependent density profile for dark matter haloes including the influence of galaxy formation

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Yang Ocean Wang

, W. P. Lin, X. Kang, Aaron Dutton

, Yu Yu, Andrea V. Macciò

Satellite Alignment. I. Distribution of Substructures and Their Dependence on Assembly History Fromn-Body Simulations

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Aaron A. Dutton

, Tommaso Treu

The bulge–halo conspiracy in massive elliptical galaxies: implications for the stellar initial mass function and halo response to baryonic processes

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Stéphane Courteau, Michele Cappellari

, Roelof S. de Jong, Aaron A. Dutton

, Eric Emsellem, Henk Hoekstra

, L. V. E. Koopmans, Gary A. Mamon

, Claudia Maraston, Tommaso Treu, Lawrence M. Widrow

Galaxy masses

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2013 Brendon J. Brewer, Philip J. Marshall, Matthew W. Auger, Tommaso Treu, Aaron A. Dutton

, Matteo Barnabè

The SWELLS survey – VI. Hierarchical inference of the initial mass functions of bulges and discs

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Arianna Di Cintio, Chris B. Brook, Andrea V. Macciò, Greg S. Stinson, Alexander Knebe, Aaron A. Dutton

, James Wadsley

The dependence of dark matter profiles on the stellar-to-halo mass ratio: a prediction for cusps versus cores

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Charlie Conroy, Aaron A. Dutton

, Genevieve J. Graves, J. Trevor Mendel, Pieter G. van Dokkum

Dynamical Versus Stellar Masses in Compact Early-Type Galaxies: Further Evidence for Systematic Variation in the Stellar Initial Mass Function

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Jeffrey A. Newman, Michael C. Cooper, Marc Davis, S. M. Faber, Alison L. Coil, Puragra Guhathakurta, David C. Koo, Andrew C. Phillips, Charlie Conroy, Aaron A. Dutton

, Douglas P. Finkbeiner, Brian F. Gerke, David J. Rosario, Benjamin J. Weiner

, C. N. A. Willmer and 19 other authors

The Deep2 Galaxy Redshift Survey: Design, Observations, Data Reduction, and Redshifts

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Aaron A. Dutton

, Andrea V. Macciò, J. Trevor Mendel, Luc Simard

Universal IMF versus dark halo response in early-type galaxies: breaking the degeneracy with the Fundamental Plane

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Xi Kang, Andrea V. Macciò, Aaron A. Dutton

The Effect of Warm Dark Matter on Galaxy Properties: Constraints From the Stellar Mass Function and the Tully-Fisher Relation

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