1. Introduction
2. Survey Description and Science Goals
2.1. Survey Description
2.2. Science Goals
3. MUSE Observations and Data Reduction
3.1. Observations
3.2. Data Reduction
4. Emission Line Selected Objects
4.1. Detection and Classification
4.2. Cross-Match with Photometric and Spectroscopic Catalogs
4.3. Stellar Masses
4.4. Final Emission Line Catalogs
4.5. Cross-Match with Other Multi Wavelength Catalogs
5. Spectroscopy and Identification of Photometrically Selected Objects
5.1. Field Map
5.2. Optimal 3D Spectral Extraction
5.3. Identification of Galaxies Brighter than 24th Magnitude
6. Conclusions and Outlook