Using 341 X-ray-selected AGN, this study calibrates the [Ne v] lambda3427 line as a tracer of black-hole accretion power, finding a 43% detection rate and no strong dependence on obscuration, black-hole mass, or Eddington ratio.
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BASS XLVIII: [Ne v] {\lambda}3427 Emission in Powerful Nearby Active Galactic Nuclei
Using 341 X-ray-selected AGN, this study calibrates the [Ne v] lambda3427 line as a tracer of black-hole accretion power, finding a 43% detection rate and no strong dependence on obscuration, black-hole mass, or Eddington ratio.