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New Indicators for AGN Power: The Correlation Between [O IV] lambda 25.89 micron and Hard X-ray Luminosity for Nearby Seyfert Galaxies
Meléndez, M; Kraemer, S B; Armentrout, B K; Deo, R P; Crenshaw, D M; et al. arXiv.org, Apr 7, 2008.You might have access to this document
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