|Title||The most luminous quasars at the golden epoch of AGN-galaxy evolution|
|Author||Dr Luca Zappacosta|
|Description||We propose to observe four hyper-luminous (L_IR > 10^14 Lsun), dust-reddened, type 1 quasars at z=2-3.5, recently discovered in the wide-area UKIDSS and WISE surveys. We will constrain their X-ray luminosity and, through available multiwavelength data, accurately model their SED disentangling the disk and corona contribution to such extreme bolometric luminosities.|
|Publication||The WISSH quasars project. III. X-ray properties of hyper-luminous quasars . Martocchia, S., Piconcelli, E., et all. . A&A . 608-51 . 2017 . 2017A&A...608A..51M ,
The WISSH quasars project. VII. The impact of extreme radiative field in the accretion disc and X-ray corona interplay . Zappacosta, L., Piconcelli, E., et all. . A&A . 635-5 . 2020 . 2020A&A...635L...5Z ,
|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, 2017-02-16T23:00:00Z, 076316, 17.56_20190403_1200. https://doi.org/10.5270/esa-1qwxz5t|