Galaxy Clustering Tutorial
==========================

This tutorial shows how to compute galaxy clustering statistics from halo properties using the Halo Occupation Distribution (HOD) framework.

Learning Objectives
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- Understand the halo model for galaxy clustering
- Compute halo-halo correlation functions
- Apply HOD models
- Calculate observable galaxy clustering (:math:`\xi_{gg}(r)` and :math:`w_p(r_p)`)

Overview
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The halo model connects dark matter halos to observable galaxies through:

1. **Halo Mass Function**: :math:`\phi(M)` - abundance of halos
2. **Halo Clustering**: :math:`\xi_{hh}(r, M)` - spatial distribution
3. **HOD**: Occupation of galaxies within halos
4. **Galaxy Clustering**: :math:`\xi_{gg}(r)` - observable correlation function

Coming soon: More detailed content for this tutorial.