Sereno, MauroMauroSereno2020-03-162020-03-1620150035-8711http://hdl.handle.net/20.500.12386/23301The measurement of the mass of clusters of galaxies is crucial for their use in cosmology and astrophysics. Masses can be efficiently determined with weak lensing (WL) analyses. I compiled literature catalogues of WL clusters (LC<SUP>2</SUP>). Cluster identifiers, coordinates, and redshifts have been standardized. WL masses were reported to over-densities of 2500, 500, 200, and to the virial one in the reference ΛCDM model. Duplicate entries were carefully handled. I produced three catalogues: LC<SUP>2</SUP>-single, with 485 unique groups and clusters analysed with the single-halo model; LC<SUP>2</SUP>-substructure, listing substructures in complex systems; LC<SUP>2</SUP>-all, listing all the 822 WL masses found in the literature. The catalogues and future updates are publicly available at http://pico.bo.astro.it/∼sereno/CoMaLit/LC2/.STAMPAenArticle10.1093/mnras/stu25052-s2.0-84938150845000360824000021https://academic.oup.com/mnras/article/450/4/3665/989476http://arxiv.org/abs/1409.5435v22015MNRAS.450.3665SFIS/05 - ASTRONOMIA E ASTROFISICA