A dataset provided by the European Space Agency

Name: Extremely Luminous, Heavily Obscured WISE-Selected AGN
Published: 2017-06-09T22:00:00Z

Proposal ID	078367
Title	Extremely Luminous, Heavily Obscured WISE-Selected AGN
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783670101
DOI	https://doi.org/10.5270/esa-ocxy81x
Principal Investigator, PI	Dr Daniel Stern
Abstract	The all-sky mid-IR wise mission is an extremely efficient black hole finder,identifying vast numbers of AGN, including the rarest, most luminous, mostobscured AGN. {bf In AO14 we were awarded a 20~ks Priority B observation ofWISE~J2246-0526, the most luminous galaxy currently known, but the observationswere essentially useless due to strong flaring.} We propose to re-observe thatsource in AO15. in order to measure its high-energy properties and columndensities.
Publications	Heavy X-ray obscuration in the most luminous galaxies discovered by WISE \|Vito F. Brandt W. N. et al. \| MNRAS \| 474-4528 \| 2018 \| 2018MNRAS.474.4528V \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.474.4528V 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	2016-05-17T22:58:04Z/2016-05-18T06:44:44Z
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	2017-06-09T22:00:00Z
Keywords	"luminous galaxy", "energy properties", "obscured agn", "flaring .}", "column densities", "efficient blackhole finder", "heavily obscured wise", "j2246 0526"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Daniel Stern, 2017, 'Extremely Luminous, Heavily Obscured WISE-Selected AGN', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ocxy81x