1. INTRODUCTION

2. THE PINES SURVEY
2.1. Observing Facility and Instrument
2.2. Target Sample
2.3. Observational Strategy
2.4. Guiding Performance
2.5. Log Files

3. THE PINES PHOTOMETRIC PIPELINE
3.1. Calibration Images
3.2. Bad Pixel Identification and Data Reduction
3.3. Target and Reference Identification
3.4. Astrometric Solution and Source Spectral Types
3.5. Centroiding
3.6. Aperture Photometry and Bad Pixel Correction
3.7. Light Curves
3.8. Precipitable Water Vapor (PWV) Corrections

4. PHOTOMETRIC PERFORMANCE AND FIRST RESULTS
4.1. Photometric Performance
4.2. Recovery of a Transit of WASP-2 b
4.3. Recovered Variables
4.4. New Variable: WISE J045746.08-020719.2