A dataset provided by the European Space Agency

Name: Hyperluminous Quasars at z=2-3 Caught in the Radiative Feedback Phase
Published: 2016-01-13T23:00:00Z

Proposal ID	074532
Title	Hyperluminous Quasars at z=2-3 Caught in the Radiative Feedback Phase
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0745320101
DOI	https://doi.org/10.5270/esa-ahi8erk
Principal Investigator, PI	Dr Manda Banerji
Abstract	We have recently used XMM-Newton observations to directly detect a powerfulquasar in a heavily dust-shrouded galaxy at z=2.5. This dusty quasar:ULASJ1234+0907, is observed in the AGN blowout phase and is among the mostluminous X-ray quasars known (LX~1E45 erg/s). Following these observations, wehave now spectroscopically confirmed two new extremely red, dusty broad-linequasars at z~2.5 with similarly extreme properties to ULASJ1234+0907. We proposeto obtain X-ray spectra of these in order to investigate the physical propertiesof the absorbing material and test models of radiative feedback on dust duringthe main epoch of galaxy formation and accretion activity in the Universe.
Publications	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 A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies \|Ojha Vineet Chand Hum et al. \| ApJ \| 896-95 \| 2020 \| 2020ApJ...896...95O \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...95O 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	2014-12-16T12:09:24Z/2014-12-17T03:59:24Z
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	2016-01-13T23:00:00Z
Last Update	2025-01-27
Keywords	"agn blowout phase", "absorbing material", "main epoch", "accretion activity", "xmm newton", "galaxy formation", "radiative feedback phase", "1e45 erg", "XMM-Newton", "test models", "dusty quasar", "radiative feedback", "XMM", "luminous xray quasars", "powerful quasar", "hyperluminous quasars", "xray spectra", "physical properties"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Manda Banerji, 2016, 'Hyperluminous Quasars at z=2-3 Caught in the Radiative Feedback Phase', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ahi8erk