TL;DR
This paper introduces the GRAND-HOD framework, a generalized and differentiable halo occupation distribution model, to analyze galaxy correlation functions and improve understanding of galaxy-halo connections.
Contribution
The paper develops a flexible, generalized HOD model incorporating various physics and biases, and demonstrates its effectiveness in analyzing 2PCF and squeezed 3PCF data.
Findings
Degeneracies in projected 2PCF are broken in redshift-space and squeezed 3PCF.
Squeezed 3PCF provides additional constraints on galaxy-halo models.
Current HOD framework predicts squeezed 3PCF with high accuracy.
Abstract
We present the GeneRalized ANd Differentiable Halo Occupation Distribution (GRAND-HOD) routine that generalizes the standard 5 parameter halo occupation distribution model (HOD) with various halo-scale physics and assembly bias. We describe the methodology of 4 different generalizations: satellite distribution generalization, velocity bias, closest approach distance generalization, and assembly bias. We showcase the signatures of these generalizations in the 2-point correlation function (2PCF) and the squeezed 3-point correlation function (squeezed 3PCF). We identify generalized HOD prescriptions that are nearly degenerate in the projected 2PCF and demonstrate that these degeneracies are broken in the redshift-space anisotropic 2PCF and the squeezed 3PCF. We also discuss the possibility of identifying degeneracies in the anisotropic 2PCF and further demonstrate the extra constraining…
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