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- W1968656069 abstract "We report a sizable class of type 1 active galactic nuclei (AGNs) with unusually weak near-infrared (1-3{mu}m) emission in the XMM-COSMOS type 1 AGN sample. The fraction of these hot-dust-poor AGNs increases with redshift from 6% at lowredshift (z < 2) to 20% at moderate high redshift (2 < z < 3.5). There is no clear trend of the fraction with other parameters: bolometric luminosity, Eddington ratio, black hole mass, and X-ray luminosity. The 3{mu}m emission relative to the 1{mu}m emission is a factor of 2-4 smaller than the typical Elvis et al. AGN spectral energy distribution (SED), which indicates a torus covering factor of 2%-29%, a factor of 3-40 smaller than required by unified models. The weak hot dust emission seems to expose an extension of the accretion disk continuum in some of the source SEDs. We estimate the outer edge of their accretion disks to lie at $(0.3-2.0) /times 10^4$ Schwarzschild radii, ~10-23 times the gravitational stability radii. Formation scenarios for these sources are discussed." @default.
- W1968656069 created "2016-06-24" @default.
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- W1968656069 date "2010-10-29" @default.
- W1968656069 modified "2023-10-01" @default.
- W1968656069 title "HOT-DUST-POOR TYPE 1 ACTIVE GALACTIC NUCLEI IN THE COSMOS SURVEY" @default.
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- W1968656069 doi "https://doi.org/10.1088/2041-8205/724/1/l59" @default.
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