ESO DOI Service

• Prandoni, Isabella [INAF–Institute of Radio Astronomy, Bologna, Italy]
• Sargent, Mark [International Space Science Institute, Bern, Switzerland]
• Adams, Elizabeth A. K. [Kapteyn Astronomical Institute, University of Groningen, the Netherlands; ASTRON, the Netherlands Institute for Radio Astronomy, Dwingeloo, the Netherlands]
• Catinella, Barbara [International Centre for Radio Astronomy Research, The University of Western Australia, Crawley, Australia; Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Australia]
• Cirasuolo, Michele [European Southern Observatory (ESO)]
• Emsellem, Eric [European Southern Observatory (ESO); ENS de Lyon, CNRS, Lyon Astrophysics Research Centre, University of Lyon, France]
• Hopkins, Andrew [School of Mathematical and Physical Sciences, Macquarie University, New South Wales, Australia]
• Maddox, Natasha [School of Physics, H.H. Wills Physics Laboratory, University of Bristol, UK]
• Mainieri, Vincenzo [European Southern Observatory (ESO)]
• Wisnioski, Emily [Research School of Astronomy and Astrophysics, Australian National University, Canberra, Australia; Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Australia]
• Colless, Matthew [Research School of Astronomy and Astrophysics, Australian National University, Canberra, Australia]

We highlight the potential benefits of a synergistic use of SKAO and ESO facilities for galaxy evolution studies, focusing on the role that ESO spectroscopic surveys can play in supporting next-generation radio continuum and atomic hydrogen (HI) surveys. More specifically we illustrate the role that currently available or soon to be operational ESO multiplex spectrographs can play for three classes of projects: large/deep redshift survey campaigns, integral field unit/Atacama Large Millimeter/submillimeter Array (IFU/ALMA) surveys of selected regions of sky, and IFU/ALMA follow-ups of selected samples. We conclude with some general recommendations for an efficient joint exploitation of ESO–SKAO surveys.