Astronomy and Astrophysics – Astronomy
Scientific paper
May 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987nascp2466..727m&link_type=abstract
Star formation in galaxies, Proceedings of a conference at the California Institute of Technology, Pasadena, California, June 16
Astronomy and Astrophysics
Astronomy
Active Galactic Nuclei, Infrared Spectra, Spectral Energy Distribution, Star Formation, Thermal Emission, Ultraviolet Spectra, Absorption Spectra, Infrared Astronomy, Line Spectra, Luminous Intensity, Seyfert Galaxies, Stellar Spectrophotometry
Scientific paper
Data 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.
Edelson Richard A.
Malkan Matthew A.
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