1 To fill in the missing pieces in studying the evolution of large-scale outflows over the past 8 billion years (at z<1.0) that were left incomplete in our previous TRF project.
2 To enhance the sample of blobs at z>1.0. This will significantly improve the statistics of our studies, as the new survey covers a remarkably larger area than before.
3 To understand the evolution of AGN/stellar feedback and subsequent quenching process that turns star-forming galaxies into passively evolving elliptical galaxies.
4 To request telescope time for spectroscopic follow-up observations, which could lead to understanding of the physical mechanisms behind galactic-scale outflows of gas.
