The Power of Deconvolution for Study of QSO Host Galaxies

Details The Power of Deconvolution for Study of QSO Host Galaxies The Power of Deconvolution for Study of QSO Host Galaxies

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010iaus..267..117l&link_type=abstract

Co-Evolution of Central Black Holes and Galaxies, Proceedings of the International Astronomical Union, IAU Symposium, Volume 267

Statistics

Applications

Techniques: Image Processing, Spectroscopy, Galaxies: Active, Quasars: General

Scientific paper

The major challenge in studying QSO host galaxies is to remove the QSO contribution, which often outshines the whole system. Our group has acquired the technical ability to handle such data, for images and slit spectroscopy, as well as integral field spectroscopy. We review here the major techniques developed by our team, and their latest applications. We are open for collaboration with other teams to spread the use of these powerful techniques.

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