I am mainly interested in how today’s most massive galaxies form and evolve. In particular, by studying their structure, star formation, clustering properties as well as AGN activities at the peak epoch of the cosmic star formation history (z ~ 1-4), I aim to better constrain the formation mechanisms of massive galaxies during the first half of the universe’s age.
My main activities within the ASTRODEEP consortium are to better de-confuse Herschel (SPIRE) images, produce new Herschel catalogs and identify distant (dusty) galaxies.
Email: tao.wang@cea.fr