2 MULTI-WAVELENGTH DATA  
2.1 S2CLS  
2.2 Ancillary data  

3 SOURCE IDENTIFICATION  
3.1 Counterpart matching  
3.2 Reliability of galaxy identifications  

4 DERIVED PROPERTIES  
4.1 Redshift distribution  
4.2 IR luminosities, SFRs, & dust properties  

5 CONCLUSIONS