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The spectral energy distribution (SED) modeling and fitting is the principal technique for the determination of fundamental galaxy parameters, such as its stellar mass and star formation rate (SFR).However, the accuracy of the derived parameters is sensitive to the models being used and the assumed Bayesian priors.

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In an engaging showcase of interdisciplinary collaboration, Professor Songhu Wang from the Astronomy Department, Megan Young, Lecturer and Digital Art Area Head at the Eskenazi School of Art, Architecture + Design, and Ji Yeon Kim, Associate Professor of Music in Guitar at the Jacobs School of Music, have merged their expertise to create a distinctive experience that blends music, digital art, and astrophysics.

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