A top-heavy IMF in stellar population models can reduce inferred masses of bright JWST galaxies by an order of magnitude, quantified by a new exponential fit.
@doi [ ] 10.1086/168721, https://ui.adsabs.harvard.edu/abs/1990ApJ...354..644B 354
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Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation
A top-heavy IMF in stellar population models can reduce inferred masses of bright JWST galaxies by an order of magnitude, quantified by a new exponential fit.