X-ray monitoring of the radio and gamma-ray loud Narrow-Line Seyfert 1
  Galaxy PKS 2004-447
  We present preliminary results of the X-ray analysis of XMM-Newton and Swift
observations as part of a multi-wavelength monitoring campaign in 2012 of the
radio-loud narrow line Seyfert 1 galaxy PKS 2004-447. The source was recently
detected in gamma-rays by Fermi/LAT among only four other galaxies of that
type. The 0.5-10 keV X-ray spectrum is well-described by a simple absorbed
powerlaw (photon index ~ 1.6). The source brightness exhibits variability on
timescales of months to years with indications for spectral variability, which
follows a 'bluer-when-brighter' behaviour, similar to blazars.
