Constraining clumpy dusty torus models using optimized filter sets
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/428/1/195/3559950/195.pdf
Reference40 articles.
1. TORUS AND ACTIVE GALACTIC NUCLEUS PROPERTIES OF NEARBY SEYFERT GALAXIES: RESULTS FROM FITTING INFRARED SPECTRAL ENERGY DISTRIBUTIONS AND SPECTROSCOPY
2. LOCAL LUMINOUS INFRARED GALAXIES. II. ACTIVE GALACTIC NUCLEUS ACTIVITY FROMSPITZER/INFRARED SPECTROGRAPH SPECTRA
3. Probing the nuclear and circumnuclear activity of NGC 1365 in the infrared
4. Unified Models for Active Galactic Nuclei and Quasars
5. BayesCLUMPY: BAYESIAN INFERENCE WITH CLUMPY DUSTY TORUS MODELS
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1. Torus model properties of an ultra-hard X-ray selected sample of Seyfert galaxies;Monthly Notices of the Royal Astronomical Society;2019-04-10
2. SOFIA/FORCAST resolves 30–40 μm extended dust emission in nearby active galactic nuclei;Monthly Notices of the Royal Astronomical Society;2018-12-10
3. The Emission and Distribution of Dust of the Torus of NGC 1068;The Astrophysical Journal;2018-05-29
4. On the nature of the high-energy rollover in 1H 0419-577;Monthly Notices of the Royal Astronomical Society;2018-02-09
5. Investigating the dusty torus of Seyfert galaxies using SOFIA/FORCAST photometry;Monthly Notices of the Royal Astronomical Society;2016-07-28
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