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Associated Absorption at Low and High Redshift

Published online by Cambridge University Press:  12 April 2016

Martin Elvis ,
Smita Mathur ,
Belinda J. Wilkes ,
Fabrizio Fiore ,
Paolo Giommi  and
Paolo Padovan
Martin Elvis
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA
Smita Mathur
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA
Belinda J. Wilkes
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA
Fabrizio Fiore
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA SAX Data Center, Roma, Italy
Paolo Giommi
Affiliation:
SAX Data Center, Roma, Italy
Paolo Padovan
Affiliation:
SAX Data Center, Roma, Italy

Abstract

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Combining information on absorbing material in AGN from X-ray and the UV creates a powerful investigative tool. Here we give examples from both low and high redshift.

Type
V. Emission Lines, Absorption Lines, the Continuum, and their Relationships
Information
International Astronomical Union Colloquium , Volume 159: Emission Lines in Active Galaxies: New Methods and Techniques , 1997 , pp. 236 - 239
Copyright
Copyright © Astronomical Society of the Pacific 1997

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