The Narrow-Line Seyfert 1 galaxy IRAS13224-3809 shows strong iron-K and L broadlines and high-frequency soft X-ray time lags indicating reflection from theinnermost regions about a rapidly spinning black hole. It persistently varieswith high amplitude changes every 2 to 3 days. The peak frequency and energyspectrum of the lags varies with flux, probably due to changes in size of thecorona. We propose a Very Large Programme consisting of a 1.5Ms observation ofthis object, which will enable the full range of flux levels to be studied,yielding a dynamic picture of the changing height and size of the corona andtransforming our understanding of how luminous black hole accretion operates.
Instrument
EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage
2016-07-26T18:18:44Z/2016-08-11T08:16:32Z
Version
17.56_20190403_1200
Mission Description
The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
European Space Agency, Prof Andrew Fabian, 2016, 'Mapping the inner accretion flow: dynamic reverberation in IRAS 13224-3809', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-4hpgw43
