A dataset provided by the European Space Agency

Name: X-raying the most powerful quasars in the golden epoch of AGN-galaxy evolution
Published: 2016-03-04T23:00:00Z

Proposal ID	074501
Title	X-raying the most powerful quasars in 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=0745010101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0745010301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0745010401
DOI	https://doi.org/10.5270/esa-jzlbgfo
Principal Investigator, PI	Dr Luca Zappacosta
Abstract	We propose to observe four hyper-luminous (L_IR > 10^14 L_sun), dust-reddened,type I quasars at z=2-3, recently discovered in the wide-area UKIDSS and WISEsurveys. We will constrain their X-ray luminosity and, through availablemultiwavelength data, accurately model their SED dinsentangling the disk andcorona contribution to such extreme IR luminosities
Publications	XMM-Newton publication statistics \|Ness J.-U. Parmar A. N. et al. \| AN \| 335-210 \| 2014 \| 2014AN....335..210N \| http://ui.adsabs.harvard.edu/#abs/2014AN....335..210N The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch Eric W. \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F 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 X-ray observations of luminous dusty quasars at z > 2 \|Lansbury G. B. Banerji M. et al. \| MNRAS \| 495-2652 \| 2020 \| 2020MNRAS.495.2652L \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.495.2652L The composite X-ray spectra of radio-loud and radio-quiet SDSS quasars \|Zhou Min-Hua Gu Min-Feng \| RAA \| 21-4 \| 2021 \| 2021RAA....21....4Z \| http://ui.adsabs.harvard.edu/#abs/2021RAA....21....4Z 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 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	2014-11-14T14:25:45Z/2015-02-16T19:58:21Z
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	2016-03-04T23:00:00Z
Keywords	"xray luminosity", "multiwavelength data", "agn galaxy evolution", "ir luminosities", "dust reddened", "hyper luminous l_ir", "x raying", "powerful quasars", "wise surveys", "golden epoch", "sed dinsentangling"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Luca Zappacosta, 2016, 'X-raying the most powerful quasars in the golden epoch of AGN-galaxy evolution', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-jzlbgfo