Kreikenbohm A, Kadler M, Wilms J, Schulz R, Mueller C, Ojha R, Ros E, Mannheim K, Elsaesser D (2013)
Publication Status: Published
Publication Type: Conference contribution
Publication year: 2013
Book Volume: 61
Article Number: UNSP 04017
DOI: 10.1051/epjconf/20136104017
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 (Gamma similar to 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.
APA:
Kreikenbohm, A., Kadler, M., Wilms, J., Schulz, R., Mueller, C., Ojha, R.,... Elsaesser, D. (2013). X-ray monitoring of the radio and gamma-ray loud Narrow-Line Seyfert 1 Galaxy PKS 2004-447.
MLA:
Kreikenbohm, A., et al. "X-ray monitoring of the radio and gamma-ray loud Narrow-Line Seyfert 1 Galaxy PKS 2004-447." 2013.
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