1. Introduction

2. Data and Modeling  
2.1. The NOAO Deep Wide-Field Survey Boötes Field  
2.2. WISE Observations  
2.3. Spectral Energy Distribution Modeling  

3. WISE AGN Color Selection  
3.1. Magnitude-Independent AGN Color Selection  
3.2. Magnitude-Dependent AGN Color-Selection  
3.3. Comparison with the Literature  

4. Properties of WISE AGN Candidates  
4.1. Photometric Redshift Accuracy for WISE AGN Candidates  
4.2. Redshift Distribution of WISE AGN Candidates  
4.3. SED Analysis of WISE AGN Candidates  
4.4. Keck Observations  

5. Dust Reddening in AGN  
5.1. Sample Selection Function  
5.2. Method  
5.3. Results  

6. Conclusions