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We use field-level forward models of galaxy clustering and the EFT likelihood formalism to study, for the first time for self-consistently simulated galaxies, the relations between the linear $b_1$ and second-order bias parameters $b_2$ and $b_{K^2}$.
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G. Cabass and F. Schmidt, “The EFT likelihood for large-scale structure,” JCAP
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J. A. Peacock and R. E. Smith, “Halo occupation numbers and galaxy bias,” Mon. Not. R. Astron. Soc
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V. Springel, S. D. M. White, G. Tormen, and G. Kauffmann, “Populating a cluster of galaxies - I. Results at [formmu2]z=0,” Mon. Not. R. Astron. Soc
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A. A. Berlind, D. H. Weinberg, A. J. Benson, C. M. Baugh, S. Cole, R. Davé, C. S. Frenk, A. Jenkins, N. Katz, and C. G. Lacey, “The Halo Occupation Distribution and the Physics of Galaxy Formation,” Astrophys. J
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A. V. Kravtsov, A. A. Berlind, R. H. Wechsler, A. A. Klypin, S. Gottlöber, B. o. Allgood, and J. R. Primack, “The Dark Side of the Halo Occupation Distribution,” Astrophys. J
2004
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G. Cabass, “The EFT likelihood for large-scale structure in redshift space,” JCAP
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F. Schmidt, “Sigma-eight at the percent level: the EFT likelihood in real space,” JCAP
2009
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F. Schmidt and F. Beutler, “Imprints of reionization in galaxy clustering,” Phys. Rev. D
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V. Desjacques, D. Jeong, and F. Schmidt, “Large-scale galaxy bias,” Phys. Rep
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M. M. Abidi and T. Baldauf, “Cubic halo bias in Eulerian and Lagrangian space,” JCAP
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