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Fig. 4.

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Illustration of the SFR computation method for a given SF halo in a kth simulation snapshot at a given redshift zk. The total SFR of an object is computed by summing the SFR of the galaxies inside a cylinder of length DL(δz) and diameter Ds(θ) centred on the halo. The contributions of N background and foreground boxes along the LOS are considered by adding the mean total SFR computed inside cylinders with the same parameters DL(δz) and θ in the nearest snapshots at the lower and higher redshifts, zk − 1 and zk + 1.

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