1. Introduction

2. The Trident survey

3. Observations and data reduction
3.1. Custom filters
3.2. Data reduction
3.3. Standard stars
3.4. Archival and catalog data

4. Candidate selection

5. Warm dust properties
5.1. Comparison to previous work

6. SED fitting
6.1. Selection of SED fitting parameters
6.2. SED fitting results

7. Conclusions