Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12188/27843
Title: UV dust attenuation as a function of stellar mass and its evolution with redshift
Authors: Bogdanoska, Jana 
Denis Burgarella
Keywords: Galaxies: evolution
Galaxies: high-redshift
Cosmology: early Universe
Issue Date: Dec-2019
Publisher: Soci´et´e Francaise d’Astronomie et d’Astrophysique (SF2A) 2019
Journal: SF2A 2019 proceedings
Conference: SF2A 2019
Abstract: Describing the Universe in its early stages requires obtaining knowledge about the various components in distant galaxies (stars, gas, dust). This work aims to further constrain the relationship between the ultraviolet dust attenuation and stellar mass, as well as the evolution of the dust attenuation with redshift, by creating a three dimensional model for the dust attenuation, which uses these two galactic parameters (redshift and stellar mass). By combining data from different literature sources, we were able to compile a data set comprised of estimates of photometric redshift, stellar mass and dust attenuation calculated by the infrared excess (IRX) method, i.e. by converting the ratio of the infrared-to-ultraviolet luminosity of galaxies to ultraviolet dust attenuation. Using this result, we will be able to model and predict what the emission of galaxies at high redshifts is. This information will be useful to understand and interpret the data that the ELT will collect, especially the first imaging instruments MICADO and METIS.
URI: http://hdl.handle.net/20.500.12188/27843
DOI: 10.1093/mnras/staa1928
Appears in Collections:Faculty of Natural Sciences and Mathematics: Conference papers

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