# 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