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Dusty Galaxies: Modeling Infrared Spectra from Heavily Obscured Objects
Viola, Vincent Franklin
Viola, Vincent Franklin
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Text, Physics, Department of, Honors papers, Student research
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Abstract
We fit models to heavily obscured infrared spectra taken by the Spitzer Space Telescope and prepare them for cataloguing in the Infrared Database of Extragalactic Observables from Spitzer (IDEOS). The software we use, QUESTFIT, models the spectra using up to three extincted blackbodies (including silicate, water ice, and hydrocarbon absorption) and PAH templates. We present results from a sample of the approximately 200 heavily obscured spectra that will be present in IDEOS. We will explore some of the physical properties of the various types of dust, such as their mechanisms for emission and absorption. Based on our results, we can draw conclusions as to the nature of absorbing material surrounding the galaxies, as well as potential domination by active galactic nuclei or starbursts
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