Aim of the conference is to review the state of our understanding of galaxy evolution with an emphasis on the role of neutral hydrogen and the use of neutral hydrogen observations to probe the relevant physical processes. In addition it will focus on the particular advantage of blind surveys for unraveling the details of the role of neutral, ionised and molecular gas in galaxy evolution and the importance and relevance of gas accretion and removal processes. This will include discussing the various observational and analysis methods that are required to fully explore the data forthcoming from large surveys.

Scientific Organising Committee

Local Organising Committee

This event has received funding from the Koninklijke Nederlandse Academie van Wetenschappen, the Netherlands Research School for Astronomy, the European Union's Horizon 2020 research and innovation programme under grant agreement No 730562 [RadioNet], the Kapteyn Astronomical Institute, the Netherlands Institute for Radio Astronomy and the Leids Kerkhoven Bosscha Fund.