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- W2494494986 abstract "We report on the performance of the statistical, X-ray absorption lines identification procedure XLINE-ID. As illustration, it is used to estimate the time averaged gas density $n_H(r)$ of a representative AGN's warm absorber ($Tapprox 10^5$~K) X-ray simulated spectrum. The method relies on three key ingredients: (1) a well established emission continuum level; (2) a robust grid of photoionisation models spanning several orders of magnitude in gas density ($n_H$), plasma column density ($N_H$), and in ionization states; (3) theoretical curves of growth for a large set of atomic lines. By comparing theoretical and observed equivalent widths of a large set of lines, spanning highly ionized charge states from O, Ne, Mg, Si, S, Ar, and the Fe L-shell and K-shell, we are able to infer the location of the X-ray warm absorber." @default.
- W2494494986 created "2016-08-23" @default.
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- W2494494986 date "2016-01-01" @default.
- W2494494986 modified "2023-10-14" @default.
- W2494494986 title "X-Ray Outflows of Active Galactic Nuclei Warm Absorbers: A 900 ks Chandra Simulated Spectrum" @default.
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- W2494494986 doi "https://doi.org/10.1007/978-3-319-27965-7_28" @default.
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