DiRAC 2.5y Bridging Funding - UCL

Lead Research Organisation: University College London
Department Name: Physics and Astronomy

Abstract

Abstracts are not currently available in GtR for all funded research. This is normally because the abstract was not required at the time of proposal submission, but may be because it included sensitive information such as personal details.

Publications

10 25 50
publication icon
Dalla Vecchia C (2020) Constraining the inner density slope of massive galaxy clusters in Monthly Notices of the Royal Astronomical Society

publication icon
Soussana A (2020) The impact of AGN feedback on galaxy intrinsic alignments in the Horizon simulations in Monthly Notices of the Royal Astronomical Society

publication icon
Gratton S (2020) Understanding parameter differences between analyses employing nested data subsets in Monthly Notices of the Royal Astronomical Society

publication icon
Pagano P (2020) Effect of coronal loop structure on wave heating through phase mixing in Astronomy & Astrophysics

publication icon
Simpson C (2020) The milky way total mass profile as inferred from Gaia DR2 in Monthly Notices of the Royal Astronomical Society

publication icon
Falle S (2020) Thermal instability revisited in Monthly Notices of the Royal Astronomical Society

publication icon
Davé R (2020) Galaxy cold gas contents in modern cosmological hydrodynamic simulations in Monthly Notices of the Royal Astronomical Society

publication icon
Stevenson P (2020) A time-dependent Hartree-Fock study of triple-alpha dynamics in SciPost Physics Proceedings

publication icon
Robson D (2020) X-ray emission from hot gas in galaxy groups and clusters in simba in Monthly Notices of the Royal Astronomical Society

publication icon
Campargue A (2020) Observation of electric-quadrupole infrared transitions in water vapor in Physical Review Research

publication icon
Xu W (2020) Galaxy properties in the cosmic web of EAGLE simulation in Monthly Notices of the Royal Astronomical Society

publication icon
Pluriel W (2020) ARES. III. Unveiling the Two Faces of KELT-7 b with HST WFC3 in The Astronomical Journal

publication icon
Garzilli A (2020) Measuring the temperature and profiles of Ly a absorbers in Monthly Notices of the Royal Astronomical Society

publication icon
Vandenbroucke B (2020) CMACIONIZE 2.0: a novel task-based approach to Monte Carlo radiation transfer in Astronomy & Astrophysics

publication icon
Evans T (2020) How unusual is the Milky Way's assembly history? in Monthly Notices of the Royal Astronomical Society

publication icon
Richardson M (2020) Simulating gas kinematic studies of high-redshift galaxies with the HARMONI integral field spectrograph in Monthly Notices of the Royal Astronomical Society

publication icon
Beraldo e Silva L (2020) Geometric properties of galactic discs with clumpy episodes in Monthly Notices of the Royal Astronomical Society

publication icon
Gómez-Guijarro C (2020) How primordial magnetic fields shrink galaxies in Monthly Notices of the Royal Astronomical Society

publication icon
White S (2020) The globular cluster system of the Auriga simulations in Monthly Notices of the Royal Astronomical Society

publication icon
Barrera-Hinojosa C (2020) GRAMSES: a new route to general relativistic N -body simulations in cosmology. Part II. Initial conditions in Journal of Cosmology and Astroparticle Physics

publication icon
Iyer K (2020) The diversity and variability of star formation histories in models of galaxy evolution in Monthly Notices of the Royal Astronomical Society

publication icon
Monaco P (2020) The accuracy of weak lensing simulations in Monthly Notices of the Royal Astronomical Society

publication icon
Katz H (2020) New methods for identifying Lyman continuum leakers and reionization-epoch analogues in Monthly Notices of the Royal Astronomical Society

publication icon
Despali G (2020) The lensing properties of subhaloes in massive elliptical galaxies in sterile neutrino cosmologies in Monthly Notices of the Royal Astronomical Society

publication icon
Bastian N (2020) The globular cluster system mass-halo mass relation in the E-MOSAICS simulations in Monthly Notices of the Royal Astronomical Society