My work
Since the early days of modern cosmology, astronomers have recognized the importance of large-scale matter structuring. The physics of gravitational instability — which links primordial density fluctuations to the formation of cosmic structures — provides the foundations for the theory of galaxy and cluster evolution. However, providing a sound description of the fate of baryons that reside within large gravitational potential wells has proven challenging.
By pushing observations of the largest objects to form to higher redshifts, I strive to better understand the evolutionary pathways of massive cosmic structures. I have specialized in using ALMA, the GBT, and ACT to retrieve the characteristics of early-formed structures like protoclusters.
Below, I refer to a selection of current projects that I lead or actively contribute to.
