1. INTRODUCTION
1.1. Comparison with Other Surveys

2. PHOTOMETRY OF STARS IN THE NR FIELD

3. THE VARIABILITY OF THE PROGRAM STARS IN THE NR FIELD

4. RR LYRAE STARS
4.1. RR Lyrae stars in NR
4.2. RR Lyrae stars in LONEOS Survey

5. THE RADIAL VELOCITY DISTRIBUTION IN THE SR FIELD

6. METALLICITIES

7. THE SELECTION OF THE BLUE HORIZONTAL BRANCH (BHB) STARS IN THE NR FIELD
7.1. Selection using the (B-V)₀ vs. (u-B)K0 Plot

8. COMPARISON WITH OTHER SURVEYS
8.1. Comparison with CHSS and B2M surveys
8.2. The Ambiguous class in the present sample

9. CONCLUSION