Dr Qianjun Hang

Research summary

I am interested in how the large scale structures of the Universe are formed and evolved, and what this can tell us about our understanding of cosmology. To do this, I use statistics, such as galaxy 2-point correlation functions and cross angular power spectra between galaxies and the Cosmic Microwave Background (CMB), to analyse data from large galaxy surveys. Currently, I would like to use the DESI Legacy Survey to explore superstructures and their imprints on the CMB.

Publications

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