Four stellar-population models overpredict the 2.4–5 μm stellar continuum of quiescent compact galaxies by 0.1–0.3 mag, with the biggest excess at intermediate ages (1–5 Gyr).
K., Melchior, P., Spergel, D
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Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations
Four stellar-population models overpredict the 2.4–5 μm stellar continuum of quiescent compact galaxies by 0.1–0.3 mag, with the biggest excess at intermediate ages (1–5 Gyr).