Relativistic spectroscopy of the extreme NLS1 IRAS13224-3809.

@article{Parker2018RelativisticSO,
  title={Relativistic spectroscopy of the extreme NLS1 IRAS13224-3809.},
  author={M. Parker and W. Alston and D. Buisson and A. Fabian and J. Jiang and E. Kara and A. Lohfink and C. Pinto},
  journal={arXiv: High Energy Astrophysical Phenomena},
  year={2018}
}
  • M. Parker, W. Alston, +5 authors C. Pinto
  • Published 2018
  • Physics
  • arXiv: High Energy Astrophysical Phenomena
  • The narrow line Seyfert 1 (NLS1) IRAS 13224-3809 is the most X-ray variable active galactic nucleus (AGN), exhibiting 0.3-10 keV flux changes of over an order of magnitude within an hour. We report on the results of the 1.5 Ms 2016 XMM-Newton/NuSTAR observing campaign, which revealed the presence of a 0.24c ultra-fast outflow in addition to the well-known strong relativistic reflection. We also summarise other key results of the campaign, such as the first detection of a non-linear RMS-flux… CONTINUE READING

    Figures from this paper.

    References

    SHOWING 1-10 OF 18 REFERENCES
    Modelling the extreme X-ray spectrum of IRAS 13224−3809
    • 35
    • PDF
    The 1.5 Ms observing campaign on IRAS 13224-3809 - I. X-ray spectral analysis
    • 31
    • PDF
    Using principal component analysis to understand the variability of PDS 456
    • 15
    • PDF