FLARES yields far higher number densities and SFRs than the COSMOS-Web little red dot sample, but the comparison uses a UV magnitude cut, not the LRD color and compactness selection, so the claimed tension with the starburst model is not established.
Discovery and properties of ultra-high redshift galaxies (9 < z <12) in the jwst ero smacs 0723 field
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Evaluating the Predictive Capacity of FLARES Simulations for High Redshift "Little Red Dots"
FLARES yields far higher number densities and SFRs than the COSMOS-Web little red dot sample, but the comparison uses a UV magnitude cut, not the LRD color and compactness selection, so the claimed tension with the starburst model is not established.