Published October 16, 2026 | Version v1

CLUMPY AGN clumpy torus models (201410, τV-averaged), averaged over orientation for Galacticus

  • 1. ROR icon Carnegie Observatories

Description

Orientation-averaged spectra of the torus emission (thermal plus scattered light) from the CLUMPY library of AGN clumpy dusty torus models (Nenkova et al. 2008a, ApJ, 685, 147;  Nenkova et al. 2008b, ApJ, 685, 160). They were converted from clumpy_models_201410_tvavg.hdf5 (https://www.clumpy.org) by dataPreparation/convertCLUMPY.py in galacticusDevTools. The file tabulates λL_λ per unit AGN luminosity over the grid in N0, Y, q, σ and τV, with covering fractions and orientation-averaged escape probabilities. The CLUMPY models are by M. Nenkova, M. Sirocky, R. Nikutta, Ž. Ivezić and M. Elitzur; we thank Robert Nikutta for permission to redistribute them. Please cite Nenkova et al. (2008a,b) if you use these data.

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Additional details

Related works

Cites
Journal article: 10.1086/590482 (DOI)
Journal article: 10.1086/590483 (DOI)
Is derived from
Dataset: https://clumpy.org/ (URL)