DiRAC 2.5 - the pathway to DiRAC Phase 3
Lead Research Organisation:
University of Cambridge
Department Name: Applied Maths and Theoretical Physics
Abstract
Refer to parent proposal from Leicester - Joint reference: T2414701
Planned Impact
Refer to parent proposal from Leicester - Joint reference: T2414701
Organisations
Publications
Kulkarni G
(2017)
Large 21-cm signals from AGN-dominated reionization
in Monthly Notices of the Royal Astronomical Society
Smith M
(2018)
Supernova feedback in numerical simulations of galaxy formation: separating physics from numerics
in Monthly Notices of the Royal Astronomical Society
Elahi P
(2016)
nIFTY galaxy cluster simulations - III. The similarity and diversity of galaxies and subhaloes
in Monthly Notices of the Royal Astronomical Society
Shen S
(2017)
Chemical enrichment of stars due to accretion from the ISM during the Galaxy's assembly
in Monthly Notices of the Royal Astronomical Society
Sembolini F
(2016)
nIFTy galaxy cluster simulations - I. Dark matter and non-radiative models
in Monthly Notices of the Royal Astronomical Society
Smith M
(2019)
Cosmological simulations of dwarfs: the need for ISM physics beyond SN feedback alone
in Monthly Notices of the Royal Astronomical Society
Kulkarni G
(2016)
Models of the cosmological 21 cm signal from the epoch of reionization calibrated with Ly a and CMB data
in Monthly Notices of the Royal Astronomical Society
Nasir F
(2017)
The effect of stellar and AGN feedback on the low-redshift Lyman a forest in the Sherwood simulation suite
in Monthly Notices of the Royal Astronomical Society
Bourne M
(2019)
AGN jet feedback on a moving mesh: lobe energetics and X-ray properties in a realistic cluster environment
in Monthly Notices of the Royal Astronomical Society
Katz H
(2019)
Tracing the sources of reionization in cosmological radiation hydrodynamics simulations
in Monthly Notices of the Royal Astronomical Society