Fig. 8.

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Response of Lyman-α clustering to variations in cosmology and IGM physics according to FORESTFLOW. The top, middle, and bottom panels of the left column show the results for β, bδ, and bη, respectively, while those of the right column do so for the perpendicular modes of P3D, the parallel modes of P3D, and P1D. Blue, orange, and red lines show the response of the previous quantities to a 5% increase in As, ΩMh2, and σT, respectively, while green lines do so for a 1% increase in .
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