Image Details
Caption: Figure 6.
Fraction of LIRGs to the optically selected galaxy population with M* >3 × 10 10 M ☉ as a function of galaxy density and redshift in two stellar mass bins: M* =3 × 10 10–10 11 M ☉ (left panel), M* >10 11 M ☉ (right panel). Filled circles: X-ray detected AGN included; open circles: X-ray detected AGN excluded.
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