activity
20032020
most citedCANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey

2.2k citations · 18.2k across the 117 of their papers we have counts for

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Showing 2019Show all

12 papers · 1 filter

astro-ph.GA2019★ 12 cited

The SFR-radius connection: data and implications for wind strength and halo concentration

Lin Lin, S. M. Faber, David C. Koo +26

This paper is one in a series that explores the importance of radius as a second parameter in galaxy evolution. The topic investigated here is the relationship between star formati…

astro-ph.GA2019★ 18 cited

Local photoionization feedback effects on galaxies

Aura Obreja, Andrea V. Macciò, Benjamin Moster +5

We implement an optically thin approximation for the effects of the local radiation field from stars and hot gas on the gas heating and cooling in the N-body SPH code GASOLINE2. We…

astro-ph.GA2019★ 86 cited

NIHAO-UHD: The properties of MW-like stellar disks in high resolution cosmological simulations

Tobias Buck, Aura Obreja, Andrea V. Macciò +3

Simulating thin and extended galactic disks has long been a challenge in computational astrophysics. We introduce the NIHAO-UHD suite of cosmological hydrodynamical simulations of…

astro-ph.GA2019★ 76 cited

A model for core formation in dark matter haloes and ultra diffuse galaxies by outflow episodes

Jonathan Freundlich, Avishai Dekel, Fangzhou Jiang +5

We present a simple model for the response of a dissipationless spherical system to an instantaneous mass change at its center, describing the formation of flat cores in dark matte…

astro-ph.GA2019★ 39 cited

NIHAO XXII: Introducing black hole formation, accretion and feedback into the NIHAO simulation suite

Marvin Blank, Andrea V. Macciò, Aaron A. Dutton +1

We introduce algorithms for black hole physics, i.e., black hole formation, accretion and feedback, into the NIHAO (Numerical Investigation of a Hundred Astrophysical Objects) proj…

astro-ph.GA2019★ 4 cited

Clues to the nature of dark matter from first galaxies

Boyan K. Stoychev, Keri L. Dixon, Andrea V. Macciò +2

We use thirty-eight high-resolution simulations of galaxy formation between redshift 10 and 5 to study the impact of a 3 keV warm dark matter (WDM) candidate on the high-redshift U…