Observed 1.5-2.5 micron excess in embedded young star clusters in the FEAST galaxies that CIGALE stellar population models fail to fit, strongest for the youngest and lowest-mass clusters.
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The near infrared SED of young star clusters in the FEAST galaxies: Missing ingredients at 1-5 $\mu$m
Observed 1.5-2.5 micron excess in embedded young star clusters in the FEAST galaxies that CIGALE stellar population models fail to fit, strongest for the youngest and lowest-mass clusters.