activity
20102016
most citedParametrizing the Stellar Haloes of Galaxies

128 citations · 318 across the 5 of their papers we have counts for

collaborators

7 papers

astro-ph.GA202245 cited

A lensed radio jet at milli-arcsecond resolution I: Bayesian comparison of parametric lens models

Devon M. Powell, Simona Vegetti, J. P. McKean +3

We investigate the mass structure of a strong gravitational lens galaxy at , taking advantage of the milli-arcsecond (mas) angular resolution of very long baseline interfe…

astro-ph.GA2021

Detecting low-mass haloes with strong gravitational lensing I: the effect of data quality and lensing configuration

Giulia Despali, Simona Vegetti, Simon D. M. White +5

This paper aims to quantify how the lowest halo mass that can be detected with galaxy-galaxy strong gravitational lensing depends on the quality of the observations and the charact…

astro-ph.GA201645 cited

Red nuggets grow inside-out: evidence from gravitational lensing

Lindsay Oldham, Matt Auger, Chris Fassnacht +7

We present a new sample of strong gravitational lens systems where both the foreground lenses and background sources are early-type galaxies. Using imaging from HST/ACS and Keck/NI…

astro-ph.GA201699 cited

Gaps in globular cluster streams: giant molecular clouds can cause them too

Nicola C. Amorisco, Facundo A. Gòmez, Simona Vegetti +1

As a result of their internal dynamical coherence, thin stellar streams formed by disrupting globular clusters (GCs) can act as detectors of dark matter (DM) substructure in the Ga…

astro-ph.CO201443 cited

On the density profile of dark matter substructure in gravitational lens galaxies

Simona Vegetti, Mark Vogelsberger

We consider three extensions of the Navarro, Frenk and White (NFW) profile and investigate the intrinsic degeneracies among the density profile parameters on the gravitational lens…

astro-ph.GA2014128 cited

Parametrizing the Stellar Haloes of Galaxies

R. D'Souza, G. Kauffmann, J. Wang +1

We study the stellar haloes of galaxies out to 70-100 kpc as a function of stellar mass and galaxy type by stacking aligned and band images from a sample of 45508 galaxies…