The FLAMINGO project: cosmological hydrodynamical simulations for large-scale structure and galaxy cluster surveys
J Schaye, R Kugel, M Schaller, JC Helly… - Monthly Notices of …, 2023 - academic.oup.com
ABSTRACT We introduce the Virgo Consortium's FLAMINGO suite of hydrodynamical
simulations for cosmology and galaxy cluster physics. To ensure the simulations are …
simulations for cosmology and galaxy cluster physics. To ensure the simulations are …
DES Y3+ KiDS-1000: Consistent cosmology combining cosmic shear surveys
TMC Abbott, M Aguena, A Alarcon… - The Open Journal of …, 2023 - research.ed.ac.uk
We present a joint cosmic shear analysis of the Dark Energy Survey (DES Y3) and the Kilo-
Degree Survey (KiDS-1000) in a collaborative effort between the two survey teams. We find …
Degree Survey (KiDS-1000) in a collaborative effort between the two survey teams. We find …
The MillenniumTNG Project: the impact of baryons and massive neutrinos on high-resolution weak gravitational lensing convergence maps
We study weak gravitational lensing convergence maps produced from the MillenniumTNG
simulations by direct projection of the mass distribution on the past backwards lightcone of a …
simulations by direct projection of the mass distribution on the past backwards lightcone of a …
IllustrisTNG in the HSC-SSP: image data release and the major role of mini mergers as drivers of asymmetry and star formation
C Bottrell, HM Yesuf, G Popping… - Monthly Notices of …, 2024 - academic.oup.com
At fixed galaxy stellar mass, there is a clear observational connection between structural
asymmetry and offset from the star-forming main sequence, ΔSFMS. Herein, we use the …
asymmetry and offset from the star-forming main sequence, ΔSFMS. Herein, we use the …
The boundary of cosmic filaments
For decades, the boundary of cosmic filaments has been a subject of debate. In this work,
we determine the physically motivated radii of filaments by constructing stacked galaxy …
we determine the physically motivated radii of filaments by constructing stacked galaxy …
Simulating ionization feedback from young massive stars: impact of numerical resolution
Modelling galaxy formation in hydrodynamic simulations has increasingly adopted various
radiative transfer methods to account for photoionization feedback from young massive …
radiative transfer methods to account for photoionization feedback from young massive …
The impact of baryons on the internal structure of dark matter haloes from dwarf galaxies to superclusters in the redshift range 0 < z < 7
We investigate the redshift evolution of the concentration–mass relationship of dark matter
haloes in state-of-the-art cosmological hydrodynamic simulations and their dark-matter-only …
haloes in state-of-the-art cosmological hydrodynamic simulations and their dark-matter-only …
Prompt cusps and the dark matter annihilation signal
As the first dark matter objects gravitationally condense, a density cusp forms immediately at
every initial density maximum. Numerical simulations and theoretical arguments suggest …
every initial density maximum. Numerical simulations and theoretical arguments suggest …
The thesan project: public data release of radiation-hydrodynamic simulations matching reionization-era JWST observations
Cosmological simulations serve as invaluable tools for understanding the Universe.
However, the technical complexity and substantial computational resources required to …
However, the technical complexity and substantial computational resources required to …
Interpreting Sunyaev–Zel'dovich observations with MillenniumTNG: mass and environment scaling relations
B Hadzhiyska, S Ferraro, R Pakmor… - Monthly Notices of …, 2023 - academic.oup.com
ABSTRACT Sunyaev–Zel'dovich (SZ) measurements can dramatically improve our
understanding of the intergalactic medium and the role of feedback processes in galaxy …
understanding of the intergalactic medium and the role of feedback processes in galaxy …