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Showing 1 to 2 of 2 for “"Dust Attenuation"”.
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Insights into the nature of dust attenuation in relation to galaxy evolution from local to cosmic noon galaxies
The dust attenuation in galaxies depends on numerous processes and physical properties, such as the stellar mass, the star formation rate (SFR), the metallicity, the star formation history (SFH), and the star-dust geometry, which also involves morphology and inclination. Throughout the work in this …
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Star-forming Galaxies and Quenched Systems throughout Cosmic Time
… deep set of spectroscopy obtained by JADES. Dust, often one of the most poorly constrained parameters in SED fitting, drives the motivation for my second project. As part of the JADES survey, utilising data obtained with the *JWST*/NIRSpec Micro-Shutter Assembly, I directly explore dust …