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The fact that the spatial nonlocality of galaxy formation is controlled by some short length scale like the Lagrangian radius is the cornerstone of the bias expansion for large-scale-structure tracers.
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2014
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M. LoVerde, “Halo bias in mixed dark matter cosmologies,” Phys. Rev
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V. Desjacques, D. Jeong, and F. Schmidt, “Large-Scale Galaxy Bias,” Phys. Rept
2018
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2018
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