activity
20152024
most citedObserved versus Simulated Halo c-Mvir Relations

1 citations · 1 across the 3 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2024

Reconciling concentration to virial mass relations

Dominik Leier, Ignacio Ferreras, Andrea Negri +1

The concentration-virial mass (c-M) relation is a fundamental scaling relation within the standard cold dark matter (CDM) framework well established in numerical simulations. Ho…

astro-ph.GA2021★ 1 cited

Observed versus Simulated Halo c-Mvir Relations

Dominik Leier, Ignacio Ferreras, Andrea Negri +1

The concentration - virial mass relation is a well-defined trend that reflects the formation of structure in an expanding Universe. Numerical simulations reveal a marked correlatio…

astro-ph.GA2021

The lens SW05 J143454.4+522850: a fossil group at redshift 0.6?

Philipp Denzel, Onur Çatmabacak, Jonathan P. Coles +8

Fossil groups are considered the end product of natural galaxy group evolution in which group members sink towards the centre of the gravitational potential due to dynamical fricti…

astro-ph.GA2015

Strong Gravitational Lensing and the Stellar IMF of Early-type Galaxies

Dominik Leier, Ignacio Ferreras, Prasenjit Saha +3

Systematic variations of the IMF in early-type galaxies, and their connection with possible drivers such as velocity dispersion or metallicity, have been much debated in recent yea…

astro-ph.GA2015

Light versus dark in strong-lens galaxies: Dark matter haloes that are rounder than their stars

Claudio Bruderer, Justin I. Read, Jonathan P. Coles +4

We measure the projected density profile, shape and alignment of the stellar and dark matter mass distribution in 11 strong-lens galaxies. We find that the projected dark matter de…