|Title||X-RAY EMISSION FROM THE GRAVITATIONALLY-LENSED HIDDEN QSO IRAS F10214+4724|
|Author||Dr KAZUSHI IWASAWA|
|Description||We propose a 45 ks XMM-Newton observation of the high redshift (z=2.3) hyperluminous infrared galaxy IRAS F10214+4724. The first X-ray detection from this gravitationally-lensed object will be aimed. Previous observations strongly suggest that this object harbours a Compton-thick AGN. Weak reflected X-ray emission is expected. The inherent source-size dependency of lensing: differential magnification, offes a possible way to constrain the size of the X-ray reflection region and the contribution of the AGN to the great bolometric luminosity.|
|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, 2005-11-27T00:00:00Z, 020104, 17.56_20190403_1200. https://doi.org/10.5270/esa-pd9t0kz|