A dataset provided by the European Space Agency

Name: The most luminous quasars at the golden epoch of AGN-galaxy evolution
Published: 2017-02-16T23:00:00Z

Proposal ID	076316
Title	The most luminous quasars at the golden epoch of AGN-galaxy evolution
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763160201
DOI	https://doi.org/10.5270/esa-1qwxz5t
Principal Investigator, PI	Dr Luca Zappacosta
Abstract	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 WISEsurveys. We will constrain their X-ray luminosity and, through availablemultiwavelength data, accurately model their SED disentangling the disk andcorona contribution to such extreme bolometric luminosities.
Publications	The WISSH quasars project. III. X-ray properties of hyper-luminous quasars \|Martocchia, S., Piconcelli, E., et al. \| A&A \| 608-51 \| 2017 \| 2017A&A...608A..51M \| http://ui.adsabs.harvard.edu/#abs/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 al. \| A&A \| 635-5 \| 2020 \| 2020A&A...635L...5Z \| http://ui.adsabs.harvard.edu/#abs/2020A&A...635L...5Z Classification of 4XMM-DR9 sources by machine learning \|Zhang, Yanxia, Zhao, Yongheng, \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z X\\u2011HESS: A large sample of highly accreting serendipitous AGN under the XMM\\u2011Newton microscope \|Laurenti, M., Tombesi, F., et al. \| AN \| 344-20230053 \| 2023 \| 2023AN....34430053L \| http://ui.adsabs.harvard.edu/#abs/2023AN....34430053L The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions \|Pan, Zeyang, Qu, Zhijie, et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez, Antonio C., \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque, Pedro, Balaji, Shyam, \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2016-02-04T06:22:43Z/2016-02-04T21:47:43Z
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.
Creator Contact	https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published	2017-02-16T23:00:00Z
Keywords	"multiwavelength data", "xray luminosity", "dust reddened", "luminous quasars", "hyper luminous l_ir", "wise surveys", "bolometric luminosities", "sed disentangling", "golden epoch", "agn galaxy evolution"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Luca Zappacosta, 2017, 'The most luminous quasars at the golden epoch of AGN-galaxy evolution', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-1qwxz5t