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V. Gorjian, K. A. Cleary, R. Chary, C. R. Lawrence, M. W. Werner (JPL/Caltech)
We have obtained MIPS 24 and 70 micron photometry as well as low resolution IRS 5 to 40 micron spectra of 30 nearby Seyfert active galactic nuclei (AGN), which have a range of hydrogen column densities from Compton thin to Compton thick. We fit the spectra with a combination of AGN and starburst spectra to ascertain the contribution of each phenomenon, and correlated the results with the X-ray properties of the Seyferts.
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Bulletin of the American Astronomical Society, 37 #2
© 2005. The American Astronomical Soceity.