Satellite fractions (left) and average centrals halo mass (right) for different analyses of DESI ELGs (Rocher et al. 2023; Yu et al. 2024; Prada et al. 2025; Gao et al. 2023, 2024; Yuan et al. 2023) for the two redshift intervals analysed in this work (0.8 < z < 1.1, purple; 1.1 < z < 1.6, green). The dashed black line separates HODs and SHAM within each redshift bin. The satellite fractions are computed for subhaloes as N_satellites/(N_centrals + N_satellites). When the average halo mass for centrals is not provided, we add the halo mass with the highest probability (white symbols). In the cases from Yu et al. (2024) and Prada et al. (2025), average halo occupations are computed for 0.8 < z < 1.6.