XMM - Newton observation of the Seyfert 1 ESO 198 - G 24

We present the results from an XMM-Newton observation (January 24, 2001) of the bright Seyfert 1 galaxy ESO 198-G24 (z=0.045). We found that this Seyfert has an intrinsic 2–10 keV luminosity of about 10 erg s−1. This source shows no intrinsic absorption in addition to the Galactic absorption (NH ∼3×1020 cm−2). We found both with EPIC and RGS that this source possesses significantly steeper spectra below ∼1.5–2 keV than observed at higher X-ray energies, the so-called soft X-ray excess. The RGS spectra reveal no significant narrow absorption lines suggesting that if there is a warm absorber, it either has a relatively low column density, or a very high ionization parameter. The RGS data are well described by the combination of a power-law, a modified black body continuum, and weak relativistic lines of Oviii, and C vi Lyα. However other interpretations are not definitely excluded. The 2–10 keV energy band is well fitted by an absorbed power-law with a photon spectral index of Γ=1.77±0.04 (consistent with the typical Γ ∼1.7 found in Seyfert 1 galaxies). We found the presence of a narrow Gaussian emission line at 6.41 keV (i.e < Fexvii) with a moderate equivalent width of about 60–70 eV, and we found an upper limit for a broad component, if any, of 75 eV. We also found a weak absorption edge associated with cold iron with an optical depth of about 0.2.