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

arXiv: Astrophysics of Galaxies Pub Date : 2020-09-30 DOI:10.1051/0004-6361/202039564

P. Bergamini, P. Rosati, E. Vanzella, G. Caminha, C. Grillo, A. Mercurio, M. Meneghetti, G. Angora, F. Calura, M. Nonino, P. Tozzi

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引用次数: 9

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, Vanzella et al. 2020b), with 17.1h integration in the North-East region of the cluster, and Hubble Frontier Fields data. We spectroscopically identify 182 multiple images from 48 background sources at 0.9

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星系团MACS J0416.1−2403的高精度强透镜模型

利用星系团东北区17.1h积分的MUSE深透镜场(MDLF, Vanzella et al. 2020b)和哈勃前沿场数据，建立了星系团MACS J0416.1-2403在z=0.396处的高精度参数强透镜模型。我们从光谱上识别了182张来自48个背景源的多幅图像，这些背景源位于0.9

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