1 Introduction
2 Data
2.1 Hyper-Suprime Cam Survey
2.2 Narrow Band Filters and [OII] Emitter Sample
2.3 Random Catalog
3 Angular Correlation Function
3.1 Correlation Function Estimation
3.2 Covariance Matrix
4 Results
4.1 Setup
4.2 Power-Law Constraints
4.3 Linearly Biased Dark Matter Model
4.4 Line Luminosity and Stellar Mass Dependence of [OII]-Emitter Clustering
5 Dark Matter-[OII] Emitter Connections
5.1 Formalism of Halo Model
5.2 Halo Occupation Distribution Model for [OII] Emitters
5.3 HOD Parameter Constraints
5.4 Derived Physical Parameters for Host Halos
5.5 Comparison to a Simpler HOD
6 Summary