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?File in questo prodotto:
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