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

46 citations · 78 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.CO202046 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.CO202012 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…

astro-ph.CO202011 cited

Probing the high-z IGM with the hyperfine transition of He

Shivan Khullar, Qingbo Ma, Philipp Busch +3

The hyperfine transition of He at 3.5cm has been thought as a probe of the high-z IGM since it offers a unique insight into the evolution of the helium component of the gas…

astro-ph.CO20199 cited

Observing the redshifted 21 cm signal around a bright QSO at

Qing-Bo Ma, Benedetta Ciardi, Koki Kakiichi +3

We use hydrodynamics and radiative transfer simulations to study the 21~cm signal around a bright QSO at . Due to its powerful UV and X-ray radiation, the QSO quickly in…

astro-ph.CO2019

The Tessellation-Level-Tree: characterising the nested hierarchy of density peaks and their spatial distribution in cosmological N-body simulations

Philipp Busch, Simon D. M. White

We use the Millennium and Millennium-II simulations to illustrate the Tessellation-Level-Tree (TLT), a hierarchical tree structure linking density peaks in a field constructed by v…

astro-ph.GA2019

The globular cluster system of the Auriga simulations

Timo L. R. Halbesma, Robert J. J. Grand, Facundo A. Gómez +5

We investigate whether the galaxy and star formation model used for the Auriga simulations can produce a realistic globular cluster (GC) population. We compare statistics of GC can…