The impact of Lyman-α radiative transfer on large-scale clustering in the Illustris simulation

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Table 1

Redshift z, spatial resolution Δ, and number of LAEs considered, N_LAE, for the post-processed snapshots.

z	Resolution Δ [pkpc]	N_LAE
2.00 (f_IGM = 2 × 10⁻⁵)
high resolution	1.2	45 594

3.01 (f_IGM = 3.7 × 10⁻⁵)
high resolution	0.8	45 434
intermediate resolution	51.9	45 434

4.01 (f_IGM = 6.8 × 10⁻⁵)
high resolution	0.7	39 782

5.85 (f_IGM = 35 × 10⁻⁵)
high resolution	0.5	23 114
intermediate resolution	30.4	23 114
low resolution	121.5	23 114

Notes. We consider halos with SFR > 0.1 M_⊙ yr⁻¹ and M_h,200 > 10¹⁰ M_⊙ as LAEs. The intermediate resolution runs have a resolution similar to ZZ11 at redshift 5.85. For each redshift, we also state the average neutral fraction, f_IGM, at a characteristic hydrogen number density of 10⁻⁴ cm⁻³.

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