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astro-ph.GA2024
Spatially Resolved Galaxy-Dust Modeling with Coupled Data-Driven Priors
Jared Siegel, Peter Melchior
A notorious problem in astronomy is the recovery of the true shape and spectral energy distribution (SED) of a galaxy despite attenuation by interstellar dust embedded in the same…
astro-ph.GA2024
Inhomogeneous Dust Biases Photometric Redshifts and Stellar Masses for LSST
ChangHoon Hahn, Peter Melchior
Spectral energy distribution (SED) modeling is one of the main methods to estimate galaxy properties, such as photometric redshifts, , and stellar masses, , for extragalact…