UV-to-optical insights into the BH* model in little red dots
The discussion of 'UV-to-optical insights into the BH* Model in Little Red Dots' focuses on a highly heterogeneous sample of LRD galaxies. The paper finds that only about six percent have a statistically robust fit for the Black Hole (BH*) model. This suggests LRDs are not uniform, often showing hybrid spectra blending stellar light with AGN activity, indicating complexity and the need for more data to resolve ambiguities.