Dust properties of LIRGs and ULIRGs from the AKARI Deep Field-South
Dust properties of LIRGs and ULIRGs from the AKARI Deep Field-South
Małgorzata Bankowicz, Katarzyna Małek, Agnieszka Pollo, Veronique Buat, Denis Burgarela and Tsutomu T. Takeuchi
[Ultra] Luminous InfraRed Galaxies ([U]LIRGs) have a very high star formation rate among star forming galaxies. We model the Spectral Energy Distributions (SEDs) of galaxies from the AKARI Deep Field-South selected at 90m. Applying the CIGALE fitter to estimate their stellar mass, dust mass and dust temperatures, we found 22 LIRGs and 17 ULIRGs, which comprises 25% of our sample. We found that the majority of ULIRGs harbour Type 2 AGN, whereas LIRGs can have both AGN types.
Proceedings of the Polish Astronomical Society, vol. 4, 182-183 (2017)
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