activity
20002018
most citedThe Shape of Dark Matter Halos: Dependence on Mass, Redshift, Radius, and Formation

590 citations · 2.3k across the 33 of their papers we have counts for

collaborators

34 papers

astro-ph.GA2018★ 1 cited

Detailed modelling of the EBL along VHE γ-ray paths

A. M. Kudoda, A. Faltenbacher

Interactions between the extragalactic background light (EBL) and very high energy γ rays (VHE; E > 10 GeV) from cosmological sources alter their γ-ray spectrum. The stronger absor…

astro-ph.HE2017★ 8 cited

Effects of Spatial Fluctuations in the Extra Galactic Background Light on Hard Gamma Ray Spectra

A. M. Kudoda, A. Faltenbacher

This study investigates the impact of the fluctuations in the extra galactic background light (EBL) on the attenuation of the hard -ray spectra of distant blazars. EBL fluctuati…

astro-ph.CO2016★ 2 cited

Cosmic Web Type Dependence of Halo Clustering

J. D. Fisher, A. Faltenbacher

We use the Millennium simulation to show that halo clustering varies significantly with cosmic web type. Halos are classified as node, filament, sheet and void halos based on the e…

astro-ph.CO2015★ 8 cited

Lagrangian Methods Of Cosmic Web Classification

J. D. Fisher, A. Faltenbacher, M. S. T. Johnson

The cosmic web defines the large scale distribution of matter we see in the Universe today. Classifying the cosmic web into voids, sheets, filaments and nodes allows one to explore…

astro-ph.HE2015

Impact of the Fluctuations in the Extragalactic Background Light on the -ray Attenuation of the Quasars

Ayman M. Kudoda, Andreas Faltenbacher

This work investigates the impact of the extragalactic background light fluctuations on very high energy -ray spectra from distant Quasars. We calculate the extragalactic backgr…

astro-ph.GA2014★ 13 cited

Ram pressure statistics for bent tail radio galaxies

Zolile Mguda, Andreas Faltenbacher, Kurt van der Heyden +4

In this paper we use the MareNostrum Universe Simulation, a large scale, hydrodynamic, non-radiative simulation in combination with a simple abundance matching approach to determin…