|Title||Searching for AGN buried in starbursts|
|Author||Dr Kazushi Iwasawa|
|Description||We propose a program searching for obscured AGN in nearby bright infrared galaxies reminiscent of NGC4945, a classical example of FIR galaxies which only hard X-ray technique can probe the obscured nuclei. We selected 11 molecular-rich, intermediate luminosity galaxies from the IRAS Bright Galaxy Sample. They are strong starburst galaxies and potentially harbour active nuclei which optical technique could not be sensitive to. X-ray detection of AGN in this sample would have significant implications for the X-ray background, far-IR background and formation of black holes in the universe.|
|Publication||No observations found associated with the current proposal|
|Instrument||EMOS1, EMOS2, EPN, OM, RGS1, RGS2|
|Mission Description||The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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.
|Publisher And Registrant||European Space Agency|
|Credit Guidelines||European Space Agency, 2003-05-15T00:00:00Z, 002554, 17.56_20190403_1200. https://doi.org/10.5270/esa-pkd6h03|