We propose an XMM EPIC observation of the bright radio galaxy NGC 1316 (FornaxA) for 60 ksec. The observation have three independent goals, each offundamental importance. First, we can investigate the spatial distribution of the inverse-Compton (IC) X-ray in the NGC 1316 east lobe, to determinedistributions of the relativistic electron and the magnetic field. Secondly,the EPIC also allows us to put a tight upper limit to the current nuclearactivity, to confirm that NGC 1316 is a precious relic of past luminous AGN.Thirdly, we can accurately measure the metal abundances of the inter-stellarmedium (ISM) of an X-ray dim elliptical galaxy, using NGC 1316 as a prototype.
Instrument
EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage
2002-02-03T15:25:53Z/2002-02-04T09:15:39Z
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, Dr Naoko Iyomoto, 2003, 'Killing Three Birds with One Stone in NGC 1316 openParFornax AclosePar', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-6olls6j
