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
Viel M
(2017)
Diagnosing galactic feedback with line broadening in the low redshift Lyman-a forest
in Monthly Notices of the Royal Astronomical Society: Letters
Smith Matthew C.
(2019)
Cosmological simulations of dwarfs: the need for ISM physics beyond SN feedback alone
in Monthly Notices of the Royal Astronomical Society
Smith Matthew C.
(2017)
Supernova feedback in numerical simulations of galaxy formation: separating physics from numerics
in ArXiv e-prints
Smith M
(2019)
Cosmological simulations of dwarfs: the need for ISM physics beyond SN feedback alone
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 - II. Radiative models
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
Rorai A
(2017)
Exploring the thermal state of the low-density intergalactic medium at z = 3 with an ultrahigh signal-to-noise QSO spectrum
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
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