Different ionisation metal lines (O I, Mg II, Fe II, Si II, Ni II, Ca II, C IV, Si IV, and N V) associated with the z_abs = 2.464 ESDLA system towards QSO SDSS J1513+0352. The N V transitions are heavily contaminated with the Lyα forest and hence we could not find any robust solution for the column density tied with C IV. Hence, we only show the N V absorption profiles here without the fit. The legends as well as the assumption on sub-component redshifts and b-values are the same as in Fig. A.1.