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), with 17.1 h integration in the northeast region of the cluster, and Hubble Frontier Fields data. We spectroscopically identify 182 multiple images from 48 background sources at 0.9?

A new high-precision strong lensing model of the galaxy cluster MACS J0416.1-2403: Robust characterization of the cluster mass distribution from VLT/MUSE deep observations

Rosati P.
Secondo
;
Angora G.;
2021

Abstract

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), with 17.1 h integration in the northeast region of the cluster, and Hubble Frontier Fields data. We spectroscopically identify 182 multiple images from 48 background sources at 0.9?
2021
Bergamini, P.; Rosati, P.; Vanzella, E.; Caminha, G. B.; Grillo, C.; Mercurio, A.; Meneghetti, M.; Angora, G.; Calura, F.; Nonino, M.; Tozzi, P....espandi
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11392/2470505
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