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The Power of Deconvolution for Study of QSO Host Galaxies

Published online by Cambridge University Press:  03 June 2010

Géraldine Letawe ,
Yannick Letawe  and
Pierre Magain
Géraldine Letawe
Affiliation:
Université de Liége, Allée du 6 aout 17 4000 Liége, Belgium Email: gletawe@ulg.ac.be
Yannick Letawe
Affiliation:
Université de Liége, Allée du 6 aout 17 4000 Liége, Belgium Email: gletawe@ulg.ac.be
Pierre Magain
Affiliation:
Université de Liége, Allée du 6 aout 17 4000 Liége, Belgium Email: gletawe@ulg.ac.be
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Abstract

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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.

Keywords

techniques: image processingspectroscopygalaxies: activequasars: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S267: Co-Evolution of Central Black Holes and Galaxies , August 2009 , pp. 117
Copyright
Copyright © International Astronomical Union 2010

References

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