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
License: https://creativecommons.org/licenses/by-nc/3.0/igo

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 Search for Young Stellar Objects within 4XMM-DR13 Using CatBoost and SPE \|Ma Xiangyao Zhang Yanxia et al. \| AJ \| 168-210 \| 2024 \| 2024AJ....168..210M \| http://ui.adsabs.harvard.edu/#abs/2024AJ....168..210M New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2015-06-21T07:48:44Z/2015-09-03T01:06:22Z
Version	21.51_20241115_1113
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	2026-07-09
Keywords	"radiative feedback phase", "unobscured quasars", "blackhole growth", "XMM-Newton", "eddington ratios", "reddened quasars", "main objective", "typical extinctions", "XMM", "broad line type", "xray properties", "hard xray luminosity", "main epoch", "xmm newton", "heavily reddened quasars"
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', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-ehcr0v0
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.