activity
20122024
most citedAn excess of small-scale gravitational lenses observed in galaxy clusters

176 citations · 518 across the 14 of their papers we have counts for

collaborators

36 papers

astro-ph.GA20241 cited

The next step in galaxy cluster strong lensing: modeling the surface brightness of multiply-imaged sources

Ana Acebron, Claudio Grillo, Sherry H. Suyu +12

Overcoming both modeling and computational challenges, we present, for the first time, the extended surface-brightness distribution model of a strongly-lensed source in a complex g…

astro-ph.GA2022

Improved strong lensing modelling of galaxy clusters using the Fundamental Plane: detailed mapping of the baryonic and dark matter mass distribution of Abell S1063

Giovanni Granata

Strong gravitational lensing (SL) has emerged as a very accurate probe of the mass distribution of cluster- and galaxy-scale dark matter (DM) haloes in the inner regions of galaxy…

astro-ph.GA20212 cited

Systematic search for lensed X-ray sources in the CLASH fields

Ang Liu, Paolo Tozzi, Piero Rosati +8

We search for unresolved X-ray emission from lensed sources in the FOV of 11 CLASH clusters with Chandra data. We consider the solid angle in the lens plane corresponding to a magn…

astro-ph.GA2021

ALMA Lensing Cluster Survey: Bright [CII] 158 m Lines from a Multiply Imaged Sub- Galaxy at

Seiji Fujimoto, Masamune Oguri, Gabriel Brammer +31

We present bright [CII] 158 m line detections from a strongly magnified and multiply-imaged () sub- ( = ) Lyman-break gal…

astro-ph.GA202130 cited

ALMA Lensing Cluster Survey: a strongly lensed multiply imaged dusty system at 6

N. Laporte, A. Zitrin, R. S. Ellis +20

We report the discovery of an intrinsically faint, quintuply-imaged, dusty galaxy MACS0600-z6 at a redshift 6.07 viewed through the cluster MACSJ0600.1-2008 (=0.46). A $\sim…

astro-ph.GA202057 cited

A new high-precision strong lensing model of the galaxy cluster MACS J0416.1-2403

Pietro Bergamini, Piero Rosati, Eros Vanzella +8

We present a new high-precision parametric strong lensing model of the galaxy cluster MACS J0416.1-2403, at z=0.396, which takes advantage of the MUSE Deep Lensed Field (MDLF), wit…