[U]LIRG dust luminosity properties with two different dust emission models

[U]LIRG dust luminosity properties with two different dust emission models

Aleksander Herzig, Małgorzata Bankowicz, Katarzyna Małek and Agnieszka Pollo

We present a comparison between two dust emission models, used by the CIGALE tool fitting galaxy Spectral Energy Distributions (SEDs) for [Ultra] Luminous InfraRed Galaxies ([U]LIRGs). We focused on the dust luminosity comparison.

Proceedings of the Polish Astronomical Society, vol. 4, 184-185 (2017)

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