activity
20172024
most citedAssembly Bias and Splashback in Galaxy Clusters

87 citations · 300 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.CO2024★ 2 cited

The relation of galaxies and dark matter haloes to the filamentary cosmic web

Navdha, Philipp Busch, Simon D. M. White

We use the Millennium Simulation to study the relation of galaxies and dark matter haloes to the cosmic web. We define the web as the unique, fully connected, percolating object wi…

astro-ph.CO2022★ 9 cited

A CRASH simulation of the contribution of binary stars to the epoch of reionization

Qing-Bo Ma, Silvia Fiaschi, Benedetta Ciardi +2

We use a set of 3D radiative transfer simulations to study the effect that a large fraction of binary stars in galaxies during the epoch of reionization has on the physical propert…

astro-ph.CO2021★ 2 cited

The Boosted Potential

Jens Stücker, Raul E. Angulo, Philipp Busch

The global gravitational potential, , is not commonly employed in the analysis of cosmological simulations, since its level sets do not show any clear correspondence to the unde…

astro-ph.CO2021★ 19 cited

Investigating X-ray sources during the epoch of reionization with the 21 cm signal

Qing-Bo Ma, Benedetta Ciardi, Marius B. Eide +3

Heating of neutral gas by energetic sources is crucial for the prediction of the 21 cm signal during the epoch of reionization (EoR). To investigate differences induced on statisti…

astro-ph.CO2020★ 46 cited

Large scale simulations of H and He reionization and heating driven by stars and more energetic sources

Marius B. Eide, Benedetta Ciardi, Luca Graziani +3

We present simulations of cosmic reionization and reheating from to , investigating the role of stars (emitting soft UV-photons), nuclear black holes (BHs, with power-l…

astro-ph.CO2020★ 12 cited

Opening Reionization: Quantitative Morphology of the Epoch of Reionization and Its Connection to the Cosmic Density Field

Philipp Busch, Marius B. Eide, B. Ciardi +1

We introduce a versatile and spatially resolved morphological characterisation of binary fields, rooted in the opening transform of mathematical morphology. We subsequently apply i…