Low X-ray Luminosity Galaxy Clusters. III: Weak Lensing Mass Reconstruction at 0.18 < z < 0.70.

Abstract

This is the 3th of a series of papers on low X-ray luminosity galaxy clusters in which we present Weak Lensing Mass reconstructions based on the photometric images ... We develop a weak gravitational lensing analysis pipeline based on several public domain packages .. The Weak Lensing analysis pipeline is tested on a simulated images of a galaxy cluster field developed for the DES survey, providing a recovery of the (induced or injected) mass distribution with high ... The high quality images allow us to reconstruct the projected mass density profiles showing ... Our results indicate ...

[Low X-ray Luminosity Galaxy Clusters. III: Weak Lensing Mass Reconstruction at 0.18 \(\lt\) z \(\lt\) 0.70]Low X-ray Luminosity Galaxy Clusters. III: Weak Lensing Mass Reconstruction at 0.18 \(\lt\) z \(\lt\) 0.70 [Elizabeth J. Gonzalez, et al]
\(^{1}\) Instituto de Astronomía Teórica y Experimental (CCT Córdoba, CONICET, UNC), Laprida 854, X5000BGR, Córdoba, Argentina.
\(^{2}\) Observatorio Astronómico de Córdoba, Universidad Nacional de Córdoba, Laprida 854, X5000BGR, Córdoba, Argentina.
\(^{3}\) Consejo Nacional de Investigaciones Científicas y Técnicas, Rivadavia 1917, C1033AAJ Buenos Aires, Argentina.
\(^{4}\) Center for Gravitational Wave Astronmy, University of Texas at Brownsville, Fort Brown 80, Calvary 206, Brownsville, TX 78520, USA.
\(^{5}\) Departamento de F´ısica, Facultad de Ciencias, Universidad de La Serena, Avenida Juan Cisternas 1200, La Serena, Chile.

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dark matter – clusters: galaxies – X-rays.