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New Indicators for AGN Power: The Correlation between O IV 25.89 $\mu$m and Hard X-Ray Luminosity for Nearby Seyfert Galaxies

, , , , , , , , , and . \apj, (July 2008)
DOI: 10.1086/588807

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New Indicators for AGN Power: The Correlation between [O IV] 25.89 μm and Har

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