Four models for super-early galaxy formation predict similar galaxy bias around 7 for faint galaxies but diverge at brighter luminosities, with the primordial black hole model showing nearly constant bias while others increase to 14.
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FuGa3D computes redshift-space correlation functions and power spectra for galaxy catalogs by defining them in a model-independent space of two redshifts and angular separation, then derives real-space metrics and multipoles from the result.
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Clustering constraints on super-early galaxy formation scenarios
Four models for super-early galaxy formation predict similar galaxy bias around 7 for faint galaxies but diverge at brighter luminosities, with the primordial black hole model showing nearly constant bias while others increase to 14.