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- W3102863417 abstract "We study the correlation between the [O III]$lambda 5007$ and X-ray luminosities of local Active Galactic Nuclei (AGNs), using a complete, hard X-ray ($>10$ keV) selected sample in the Swift/BAT 9-month catalog. From our optical spectroscopic observations at the South African Astronomical Observatory and the literature, a catalog of [O III]$lambda 5007$ line flux for all 103 AGNs at Galactic latitudes of $|b|>15^circ$ is complied. Significant correlations with intrinsic X-ray luminosity ($L_{rm X}$) are found both for observed ($L_{rm [O~III]}$) and extinction-corrected ($L_{rm [O~III]}^{rm cor}$) luminosities, separately for X-ray unabsorbed and absorbed AGNs. We obtain the regression form of $L_{rm [O~III]}$ $propto L_{rm 2-10; keV}^{1.18pm0.07}$ and $L_{rm [O~III]}^{rm cor}$ $propto L_{rm 2-10; keV}^{1.16pm0.09}$ from the whole sample. The absorbed AGNs with low ($<$0.5%) scattering fractions in soft X-rays show on average smaller $L_{rm [O~III]}/L_{rm X}$ and $L_{rm [O~III]}^{rm cor}/L_{rm X}$ ratios than the other absorbed AGNs, while those in edge-on host galaxies do not. These results suggest that a significant fraction of this population are buried in tori with small opening angles. By using these $L_{rm [O~III]}$ vs. $L_{rm X}$ correlations, the X-ray luminosity function of local AGNs (including Compton thick AGNs) in a standard population synthesis model gives much better agreement with the [O III]$lambda 5007$ luminosity function derived from the Sloan Digital Sky Survey than previously reported. This confirms that hard X-ray observations are a very powerful tool to find AGNs with high completeness." @default.
- W3102863417 created "2020-11-23" @default.
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- W3102863417 date "2015-12-02" @default.
- W3102863417 modified "2023-10-01" @default.
- W3102863417 title "[O iii]<i>λ</i>5007 AND X-RAY PROPERTIES OF A COMPLETE SAMPLE OF HARD X-RAY SELECTED AGNs IN THE LOCAL UNIVERSE" @default.
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- W3102863417 doi "https://doi.org/10.1088/0004-637x/815/1/1" @default.
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