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Article / Letter to editor
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2023
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2022
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Borrow, J.
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Schaller, M.
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Schaye, J.
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Bahé, Y.M.
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Bower, R.G.
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Nobels, F.S.J.
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Altamura, E.
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Braspenning, J.R.
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Daalen, M.P. van
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Elbers, W.
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Frenk, C.S.
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Huško, F.
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Kwan, J.
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Lacey, C.G.
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Ploeckinger, S.
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Braspenning, J.R.; Schaye, J.; Borrow, J.; Schaller, M.
2023
Sensitivity of non-radiative cloud-wind interactions to the hydrodynamic solver
Article / Letter to editor
open access
2023-11-04T00:00:00Z
Borrow, J.; Schaller, M.; Bahé, Y.M.; Schaye, J.; Ludlow, A.D.; Ploeckinger, S.; ... ; Altamura, E.
2023
The impact of stochastic modelling on the predictive power of galaxy formation simulations
Article / Letter to editor
open access
Altamura, E.; Kay, S.T.; Bower, R.G.; Schaller, M.; Bahé, Y.M.; Schaye, J.; ... ; Towler, I.
2023
EAGLE-like simulation models do not solve the entropy core problem in groups and clusters of galaxies
Article / Letter to editor
open access
Kugel, R.H.; Schaye, J.; Schaller, M.; Helly, J.C.; Braspenning, J.R.; Elbers, W.; ... ; Vernon, I.
2023
FLAMINGO: calibrating large cosmological hydrodynamical simulations with machine learning
Article / Letter to editor
open access
Schaye, J.; Kugel, R.; Schaller, M.; Helly, J.C.; Braspenning, J.; Elbers, W.; ... ; Nobels, F.S.J.
2023
The FLAMINGO project: cosmological hydrodynamical simulations for large-scale structure and galaxy cluster surveys
Article / Letter to editor
open access
Bahé, Y.M.; Schaye, J.; Schaller, M.; Bower, R.G.; Borrow, J.; Chaikin, E.; ... ; Ploeckinger, S.
2022
The importance of black hole repositioning for galaxy formation simulations
Article / Letter to editor
open access
Borrow, J.; Schaller, M.; Bower, R. G.; Schaye, J.
2022
SPHENIX: smoothed particle hydrodynamics for the next generation of galaxy formation simulations
Article / Letter to editor
open access
Borrow, J.; Schaller, M.; Bower, R.G.; Schaye, J.
2021
SPHENIX: smoothed particle hydrodynamics for the next generation of galaxy formation simulations
Article / Letter to editor
open access
Borrow, J.; Schaller, M.; Bower, R.G.
2021
Inconsistencies arising from the coupling of galaxy formation sub-grid models to pressure-smoothed particle hydrodynamics
Article / Letter to editor
open access
