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
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
Meiksin A
(2017)
Gas around galaxy haloes - III: hydrogen absorption signatures around galaxies and QSOs in the Sherwood simulation suite
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
Sembolini F
(2016)
nIFTy galaxy cluster simulations - I. Dark matter and non-radiative models
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
Kimm T
(2017)
Feedback-regulated star formation and escape of LyC photons from mini-haloes during reionisation
in Monthly Notices of the Royal Astronomical Society
DeGraf C
(2017)
Black hole clustering and duty cycles in the Illustris simulation
in Monthly Notices of the Royal Astronomical Society
Costa T
(2018)
Driving gas shells with radiation pressure on dust in radiation-hydrodynamic simulations
in Monthly Notices of the Royal Astronomical Society
Henden N
(2019)
The redshift evolution of X-ray and Sunyaev-Zel'dovich scaling relations in the fable simulations
in Monthly Notices of the Royal Astronomical Society
Fiacconi D
(2018)
Galactic nuclei evolution with spinning black holes: method and implementation
in Monthly Notices of the Royal Astronomical Society