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Assessing Ultra-Cool Dwarf Contamination in Photometrically Selected High-Redshift Galaxy Samples
Ultra-cool dwarf stars (UCDs) are a common source of contamination in high-redshift galaxy searches because both populations have red colors and these early-forming galaxies can have sizes that are difficult to resolve even with space telescopes. We develop \textbf{F}oreground \textbf{C}ontamination
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