1. Introduction

2. The LOFAR LBA Sky Survey

2.1. Survey Status

3. Data Reduction

3.1. Pre-Processing Pipeline

3.2. Calibrator Pipeline

3.3. Target Pipeline: Direction-Independent

3.4. Target Pipeline: Direction-Dependent

4. Public Data Release

4.1. Mosaic Images

4.2. Source Catalogues

5. Results

5.1. Source Sizes

5.2. Sensitivity

5.3. Astrometric Precision and Accuracy

5.4. Flux Density Uncertainties

5.5. In-band Spectral Index

6. Discussion

6.1. Curved Spectra

6.2. Source Counts

6.3. Preliminary Analysis of LoLSS Stokes V Data

7. Summary