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Cited article:
R. Maiolino , A. Marconi , M. Salvati , G. Risaliti , P. Severgnini , E. Oliva , F. La Franca , L. Vanzi
A&A, 365 2 (2001) 28-36
Published online: 2001-01-15
This article has been cited by the following article(s):
351 articles | Pages:
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Determining the Dust Extinction of Gamma‐Ray Burst Host Galaxies: A Direct Method Based on Optical and X‐Ray Photometry
Y. Li, Aigen Li and D. M. Wei The Astrophysical Journal 678 (2) 1136 (2008) https://doi.org/10.1086/528734
Three-dimensional radiative transfer models of clumpy tori in Seyfert galaxies
M. Schartmann, K. Meisenheimer, M. Camenzind, et al. Astronomy & Astrophysics 482 (1) 67 (2008) https://doi.org/10.1051/0004-6361:20078907
The mid IR – hard X-ray correlation in AGN and its implications for dusty torus models
H. Horst, P. Gandhi, A. Smette and W. J. Duschl Astronomy & Astrophysics 479 (2) 389 (2008) https://doi.org/10.1051/0004-6361:20078548
New Indicators for AGN Power: The Correlation between [Oiv] 25.89 μm and Hard X‐Ray Luminosity for Nearby Seyfert Galaxies
M. Meléndez, S. B. Kraemer, B. K Armentrout, et al. The Astrophysical Journal 682 (1) 94 (2008) https://doi.org/10.1086/588807
XMM‐NewtonObservations of the Red Type 1.8 Quasar 2M1049+5837: Reflection from Cold and Warm (Ionized) Matter
B. J. Wilkes, K. A. Pounds and G. D. Schmidt The Astrophysical Journal 680 (1) 110 (2008) https://doi.org/10.1086/588039
Modeling the Dust Properties ofz∼ 6 Quasars with ART2—All‐Wavelength Radiative Transfer with Adaptive Refinement Tree
Yuexing Li, Philip F. Hopkins, Lars Hernquist, et al. The Astrophysical Journal 678 (1) 41 (2008) https://doi.org/10.1086/529364
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