1 Introduction
2 Multi-wavelength images
2.1 ALMA observations and source identifications
2.2 Optical-to-near-infrared images
2.3 Mid-infrared-to-radio images
2.4 X-ray images
3 Counterpart identification and photometry
3.1 Optical-to-near-infrared counterparts and photometry
3.2 Mid-infrared-to-radio counterparts and photometry
4 Multi-wavelength SED
4.1 Photometric redshift calculation and estimation of stellar masses
4.2 Estimation of SFRs
4.3 Optical-to-radio SED
5 Discussion
5.2 Contribution to the cosmic SFRD
5.3 Star formation properties of the ALMA detected sources
6 Summary