1. INTRODUCTION

2. UV-BRIGHT SAMPLE SELECTION

2.1. Prevalence of Massive Star-Forming Galaxies Amongst UV-Bright Galaxies at \( z>4 \)

2.2. Search Fields

2.3. Selection of the Targets for REBELS

2.4. Characteristics of the REBELS Targets

3. OBSERVATIONAL IMPLEMENTATION OF REBELS SURVEY

4. SPECTRAL SCAN RESULTS

5. SCIENCE OBJECTIVES

6. SUMMARY