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Trystan Lambert's research career is focused exclusively on extragalactic observational astronomy, exploring both low and high redshift regimes. He holds an M.Sc. from the University of Cape Town in South Africa, where he contributed to the completion of the 2MASS Redshift Survey and developed a galaxy group catalog. Subsequently, he moved to Chile to pursue his Ph.D. at Universidad Diego Portales, studying galaxies and quasars during the epoch of reionization using ALMA and DECam. Currently, he is a Research Associate at the International Centre for Radio Astronomy Research, dedicated to developing tools that identify large-scale structures in redshift surveys, specifically the Wide Area VISTA Extragalactic Survey (WAVES). This identification is crucial for mapping the distribution of dark matter in the local universe, serving as an essential testbed for current cosmological theories. Trystan Lambert's work is closely related to the UN Sustainable Development Goals.
International Centre for Radio Astronomy Research • Perth, Australia
Developing tools to identify large-scale structures in redshift surveys.
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