Degeneracies between modified gravity and baryonic physics

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Table 2

Combinations of parameters defining the hydrodynamic effects.

Simulation	cooling	t₀	ρ₀	η_SN
Vanilla	False	0	0	0
Cool star	True	8.0	0.1	0
Cool star sn	True	8.0	0.1	0.1

Notes. t₀ is a timescale in Gyr, ρ₀ is the star formation density threshold in H cm^-3, cooling turns on or off the cooling/heating term in the energy equation, and η_SN controls the fraction of stars that explode into supernovae.

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