GT - We propose to constrain the possible contributors to the complexFe-K line emission in Sy I nuclei, where these contributors include relativistically broadened disk line emission and narrow line emission originating in a torus or other dense material in the vicinity of the nucleus.
Instrument
EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage
2000-12-22T02:53:42Z/2001-12-02T04:28:47Z
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 RICHARD GRIFFITHS, 2003, 'STRONG GRAVITY AND COMPLEX FE-LINE EMISSION IN SEYFERT I NUCLEI', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-asdb4vl
