Estimating Redshift and Physical Properties of Galaxies Using Euclid Photometry
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Overview
Novel method estimates galaxy properties using broadband photometry, suggesting improved accuracy with ground-based data.
Key Points
This research aims to develop reliable methodologies for estimating the redshift and physical properties of galaxies using photometry from the Euclid Space Telescope.
Developed a property-estimation pipeline using CatBoost for regression trees.
Evaluated performance on mock datasets from Euclid and ground-based photometry.