Inner-shell 1s - 2p Soft X-ray Absorption Lines

The HULLAC atomic code is used to compute wavelengths and oscillator strengths for the 1s np inner-shell absorption lines in Li-like to F-like ions of neon, magnesium, aluminum, silicon, sulfur, argon, calcium, and iron. Many of these lines are expected to be observed in Chandra and XMM-Newton highresolution X-ray spectra of active galaxies. The new atomic data are incorporated in the ION code for spectral modeling of photoionized plasmas. The calculated spectra are subsequently compared with the spectrum of NGC 3783 and show very good agreement. The usefulness of these lines as diagnostics for the ionization state, column densities, and velocities in line-of-sight photoionized gas is called attention to. Subject headings: atomic data — atomic processes — line: formation — galaxies: active — galaxies: nuclei — X-rays: galaxies