1. Introduction

2. The final catalogue
2.1. Selection
2.2. Observations and data processing
2.3. Information in the catalogue
2.4. Calibrator density
2.5. Ionospheric coherence times as a function of baseline
2.6. LBCS flux density calibration
2.7. Signal-to-noise reproducibility in the LoTSS survey

3. Source statistics in the LBCS sample
3.1. Point sources from FIRST
3.2. Hotspots and 3CRR sources
3.3. Quasars and radio galaxies
3.4. Comparison with MWA interplanetary scintillation observations

4. Conclusion