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Article Contents

ABSTRACT

1.INTRODUCTION

2.OBSERVED SOURCE COUNTS

2.1.From surveys to counts

2.2.Low frequency surveys

2.3.Deep surveys and sub-mJy counts

2.4.High frequency surveys and counts

3.LOCAL LUMINOSITY FUNCTIONS

4.SOURCE SPECTRA AND EVOLUTION

5.EVOLUTIONARY MODELS: RADIO AGNs

5.1.Low versus high luminosities

5.2.Steep- versus flat-spectrum sources

5.3.High-z evolution

5.4.Unified evolutionary schemes

5.5.Special classes of sources

5.5.1.GHz peaked spectrum (GPS) sources

5.5.2.Late stages of AGN evolution

6.EVOLUTIONARY MODELS: STAR-FORMING GALAXIES

6.1.Star-forming, normal and sub-mm galaxies

6.2.Radio afterglows of gamma-ray bursts (GRBs)

7.THE RADIO BACKGROUND

8.SUNYAEV-ZELDOVICH EFFECTS

8.1.Sunyaev-Zeldovich (SZ) effects in galaxy clusters

8.2.Galaxy-scale Sunyaev-Zeldovich effects

9.WIDE AREA SURVEYS AND LARGE SCALE STRUCTURE

9.1.The angular correlation function and its implications

9.2.Integrated Sachs-Wolfe (ISW) effect

10.THE FUTURE

11.CONCLUSIONS

APPENDIX

REFERENCES