A dataset provided by the European Space Agency

Name: The Most Luminous Dust-Obscured Black Holes at z~2-3
Published: 2016-09-22T22:00:00Z

Proposal ID	076378
Title	The Most Luminous Dust-Obscured Black Holes at z~2-3
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763780601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763780701
DOI	https://doi.org/10.5270/esa-ehcr0v0
Principal Investigator, PI	Dr Manda Banerji
Abstract	We propose to obtain XMM-Newton observations for a complete flux-limited sampleof 7 of the most mid infra-red luminous quasars (log(L6um) > 47.5) at the mainepoch of galaxy and black-hole growth at z 2 3. The main objective is to studythe X-ray properties of a new population of hyperluminous, heavily reddenedquasars with typical extinctions of 0.5 < E(B V ) < 2.0 and which are thereforenot detectable in wide-field optical surveys. These broad-line Type 1 reddenedquasars have the expected properties - high Eddington ratios and moderatecolumn-densities - characteristic of the radiative feedback phase. We willconstrain the hard X-ray luminosity and neutral hydrogen column density andcompare them to optically selected, essentially unobscured quasars.
Publications	High-redshift Extremely Red Quasars in X-Rays \|Goulding Andy D. Zakamska Nadia L. et al. \| ApJ \| 856-4 \| 2018 \| 2018ApJ...856....4G \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...856....4G 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	2015-06-21T07:48:44Z/2015-09-03T01:06:22Z
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	2016-09-22T22:00:00Z
Last Update	2025-01-27
Keywords	"broad line type", "unobscured quasars", "reddened quasars", "main epoch", "main objective", "xmm newton", "typical extinctions", "hard xray luminosity", "radiative feedback phase", "XMM-Newton", "heavily reddened quasars", "xray properties", "blackhole growth", "XMM", "eddington ratios"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Manda Banerji, 2016, 'The Most Luminous Dust-Obscured Black Holes at z~2-3', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ehcr0v0