Hydrodynamical simulations of the galaxy population: enduring successes and outstanding challenges

RA Crain, F van de Voort - Annual Review of Astronomy and …, 2023 - annualreviews.org
We review the progress in modeling the galaxy population in hydrodynamical simulations of
the ΛCDM cosmogony. State-of-the-art simulations now broadly reproduce the observed …

Streams, substructures, and the early history of the Milky Way

A Helmi - Annual Review of Astronomy and Astrophysics, 2020 - annualreviews.org
The advent of the second data release of the Gaia mission, in combination with data from
large spectroscopic surveys, is revolutionizing our understanding of the Galaxy. Thanks to …

The chemical enrichment in the early Universe as probed by JWST via direct metallicity measurements at z ∼ 8

M Curti, F d'Eugenio, S Carniani… - Monthly Notices of …, 2023 - academic.oup.com
We analyse the chemical properties of three z∼ 8 galaxies behind the galaxy cluster
SMACS J0723. 3-7327, observed as part of the Early Release Observations programme of …

AbacusSummit: a massive set of high-accuracy, high-resolution N-body simulations

NA Maksimova, LH Garrison… - Monthly Notices of …, 2021 - academic.oup.com
We present the public data release of the AbacusSummit cosmological N-body simulation
suite, produced with the Abacus N-body code on the Summit supercomputer of the Oak …

An atlas of color-selected quiescent galaxies at z> 3 in public JWST fields

F Valentino, G Brammer, KML Gould… - The Astrophysical …, 2023 - iopscience.iop.org
We present the results of a systematic search for candidate quiescent galaxies in the distant
universe in 11 JWST fields with publicly available observations collected during the first 3 …

A non-linear solution to the S8 tension?

A Amon, G Efstathiou - Monthly Notices of the Royal …, 2022 - academic.oup.com
Weak galaxy lensing surveys have consistently reported a lower amplitude for the matter
fluctuation spectrum, as measured by the S 8 parameter, than expected in the ΛCDM …

CEERS key paper. III. The diversity of galaxy structure and morphology at z= 3–9 with JWST

JS Kartaltepe, C Rose, BN Vanderhoof… - The Astrophysical …, 2023 - iopscience.iop.org
We present a comprehensive analysis of the evolution of the morphological and structural
properties of a large sample of galaxies at z= 3–9 using early James Webb Space …

The camels project: Cosmology and astrophysics with machine-learning simulations

F Villaescusa-Navarro, D Anglés-Alcázar… - The Astrophysical …, 2021 - iopscience.iop.org
The CAMELS Project: Cosmology and Astrophysics with Machine-learning Simulations -
IOPscience This site uses cookies. By continuing to use this site you agree to our use of cookies …

First results from the TNG50 simulation: the evolution of stellar and gaseous discs across cosmic time

A Pillepich, D Nelson, V Springel… - Monthly Notices of …, 2019 - academic.oup.com
We present a new cosmological, magnetohydrodynamical simulation for galaxy formation:
TNG50, the third and final instalment of the IllustrisTNG project. TNG50 evolves 2× 21603 …

The MillenniumTNG Project: the hydrodynamical full physics simulation and a first look at its galaxy clusters

R Pakmor, V Springel, JP Coles, T Guillet… - Monthly Notices of …, 2023 - academic.oup.com
Cosmological simulations are an important theoretical pillar for understanding non-linear
structure formation in our Universe and for relating it to observations on large scales. In …