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Infrared-ultraviolet spectra of active galactic nucleiData from IRAS and IUE were combined with ground based optical and infrared spectrophotometry to derive emission line free spectral energy distributions (SEDs) for 29 active galactic nuclei (AGNs) between 0.1 and 100 microns. The IRAS data were scaled down to account for extended emission. These correction factors, determined by comparing small aperture ground based 10.6 micron data with large aperture IRAS 12 micron fluxes, were usually less than 25%. These corrected SEDs are shown.
Document ID
19870014939
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Malkan, M. A. (California Univ. Los Angeles, CA, United States)
These corrected SEDs are shown. (California Univ. Los Angeles, CA, United States)
Date Acquired
September 5, 2013
Publication Date
May 1, 1987
Publication Information
Publication: NASA, Washington Star Formation in Galaxies
Subject Category
Astronomy
Accession Number
87N24372
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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