3.7k citations · 32.7k across the 236 of their papers we have counts for
237 papers
KURVS: The outer rotation curve shapes and dark matter fractions of star-forming galaxies
Annagrazia Puglisi, Ugnė Dudzevičiūtė, Mark Swinbank +14
We present first results from the KMOS Ultra-deep Rotation Velocity Survey (KURVS), aimed at studying the outer rotation curves shape and dark matter content of 22 star-forming gal…
The impact and response of minihalos and the inter-halo medium on cosmic reionization
Tsang Keung Chan, Alejandro Benitez-Llambay, Tom Theuns +2
An ionization front (I-front) that propagates through an inhomogeneous medium is slowed down by self-shielding and recombinations. We perform cosmological radiation hydrodynamics s…
EAGLE-like simulation models do not solve the entropy core problem in groups and clusters of galaxies
Edoardo Altamura, Scott T. Kay, Richard G. Bower +5
Recent high-resolution cosmological hydrodynamic simulations run with a variety of codes systematically predict large amounts of entropy in the intra-cluster medium at low redshift…
A sparse regression approach for populating dark matter halos and subhalos with galaxies
M. Icaza-Lizaola, Richard G. Bower, Peder Norberg +2
We use sparse regression methods (SRM) to build accurate and explainable models that predict the stellar mass of central and satellite galaxies as a function of properties of their…
The importance of black hole repositioning for galaxy formation simulations
Yannick M. Bahé, Joop Schaye, Matthieu Schaller +6
Active galactic nucleus (AGN) feedback from accreting supermassive black holes (SMBHs) is an essential ingredient of galaxy formation simulations. The orbital evolution of SMBHs is…
Smoothed Particle Radiation Hydrodynamics: Two-Moment method with Local Eddington Tensor Closure
T. K. Chan, Tom Theuns, Richard Bower +1
We present a new radiative transfer method (SPH-M1RT) that is coupled dynamically with smoothed particle hydrodynamics (SPH). We implement it in the (task-based parallel) SWIFT gal…