Multiwavelength XMM-Newton observations of the Laor et al. sample of PG quasars

C. Brocksopp, R.L.C. Starling, P. Schady, K.O. Mason, E. Romero-Colmenero, E. M. Puchnarewicz

Research output: Contribution to journalArticlepeer-review

34 Citations (Scopus)

Abstract

We present XMM-Newton/EPIC spectra for the Laor et al. sample of Palomar Green (PG) quasars. We find that a power law provides a reasonable fit to the 2–5 keV region of the spectra. Excess soft X-ray emission below 2 keV is present for all objects, with the exception of those known to contain a warm absorber. However, a single power law is a poor fit to the 0.3–10.0 keV spectrum and instead we find that a simple model, consisting of a broken power law (plus an iron line), provides a reasonable fit in most cases. The equivalent width of the emission line is constrained in just 12 objects but with low (<2σ) significance in most cases. For the sources whose spectra are well fitted by the broken-power-law model, we find that various optical and X-ray line and continuum parameters are well correlated; in particular, the power-law photon index is well correlated with the FWHM of the Hβ line and the photon indices of the low- and high-energy components of the broken power law are well correlated with each other. These results suggest that the 0.3–10 keV X-ray emission shares a common (presumably non-thermal) origin, as opposed to suggestions that the soft excess is directly produced by thermal disc emission or via an additional spectral component. We present XMM-Newton Optical Monitor (OM) data, which we combine with the X-ray spectra so as to produce broad-band spectral energy distributions (SEDs), free from uncertainties due to long-term variability in non-simultaneous data. Fitting these optical—UV spectra with a Comptonized disc model indicates that the soft X-ray excess is independent of the accretion disc, confirming our interpretation of the tight correlation between the hard and soft X-ray spectra.
Original languageEnglish
Pages (from-to)953-968
Number of pages16
JournalMonthly Notices of the Royal Astronomical Society
Volume366
Issue number3
DOIs
Publication statusPublished - 1 Mar 2006

Keywords

  • galaxies: active, quasars: general, X-rays: galaxies, Astrophysics

Fingerprint Dive into the research topics of 'Multiwavelength <i>XMM-Newton</i> observations of the Laor et al. sample of PG quasars'. Together they form a unique fingerprint.

Cite this