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Abundance of damped Lyman α absorbers in cosmological smoothed particle hydrodynamics simulations

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Table 1. Simulations employed in this study. The box-size is given in unitsof h−1 Mpc, Np is the particle number of dark matter and gas (hence ×2),mDM and mgas are the masses of dark matter and gas particles in units ofh−1 M⊙, respectively, ϵ is the comovi
Figure 1. Evolution of the total neutral hydrogen mass density in each simulation box as a function of redshift
Figure 2. Comoving DLA cross-section σ DLA as a function of total halo mass at z = 3 for the Q-, D- and G-series
Figure 3. Same as in Fig. 2, but for z = 4.5. Here, instead of G4 and G5, we show results for R3 and R4
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