Science Interests Formation of galaxies and black holes in the early universe and
their growth over cosmic time; large surveys with Hubble and other telescopes to discover new populations of distant galaxies and black holes; physical properties of active galactic nuclei using observations from radio, infrared, optical, ultraviolet through to X-ray energies.
Not exact matches
This finding provides important insights on the
growth of supermassive black holes
over cosmic time.
He continues, «We hope to expand our research to farther expanses of the universe by utilizing the superb capability of ALMA to help us understand comprehensively the
growth of supermassive black holes
over cosmic time.»
Abstract: A key goal of the Stage IV dark energy experiments Euclid, LSST and WFIRST is to measure the
growth of structure with
cosmic time from weak lensing analysis
over large regions of the sky.
Weak lensing cosmology will be challenging: in addition to highly accurate galaxy shape measurements, statistically robust and accurate photometric redshift (photo - z) estimates for billions of faint galaxies will... ▽ More A key goal of the Stage IV dark energy experiments Euclid, LSST and WFIRST is to measure the
growth of structure with
cosmic time from weak lensing analysis
over large regions of the sky.