The Long Baseline Array is an array of radio telescopes using the technique of Very Long Baseline Interferometry to achieve milli-arcsecond-scale angular resolution. The core telescopes are located in Australia, with telescopes in New Zealand and South Africa also participating regularly. In this paper the capabilities of the Long Baseline Array are described, and examples of the science undertaken with the array are given.

ABSTRACT
1. INTRODUCTION
2. A BRIEF HISTORY
3. THE TELESCOPES
4. DATA RECORDING
5. CORRELATION
6. eVLBI
7. SPACE VLBI
8. SCIENCE
9. CONCLUSION
REFERENCES

• Philip G. Edwards(CSIRO Astronomy and Space Science)
• Chris Phillips(CSIRO Astronomy and Space Science)