Metal content of the circumgalactic medium around star-forming galaxies at z ∼ 2.6 as revealed by the VIMOS Ultra-Deep Survey

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Fig. 2.

Projected angular separation (θ) amongst galaxy foreground–background galaxy pairs, axial ratio (q), effective radius (r_eff), and azimuthal angle (ϕ) distributions of the star-forming (foreground) galaxies used in our analyses. The morphological parameters were obtained from the parametric measures of Ribeiro et al. (2016), see Sect. 2 for details.

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