1. INTRODUCTION
2. THE DATA SAMPLE
2.1. Wavelet-based Detection of $24\mu\mathrm{m}$ Sources
2.2. The Lockman Hole Source Sample
2.3. Empirical Redshift Distributions
3. CLUSTERING PROPERTIES OF $24\;\mu\mathrm{m}$ SELECTED GALAXIES
4.1. Galaxy Population Model
4.2. Halo Mass and Number Density
4.3. Full Limber Modeling of the Observed Angular Correlation Function
5. COMPARISON WITH PREVIOUS MEASUREMENTS
6. CONCLUSIONS
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