A dataset provided by the European Space Agency

Name: COMPTON THICK AGN: THE PHYSICS BEHIND THE OBSCURATION
Published: 2018-11-21T23:00:00Z

Proposal ID	079568
Title	COMPTON THICK AGN: THE PHYSICS BEHIND THE OBSCURATION
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0795680101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0795680201
DOI	https://doi.org/10.5270/esa-4gxa6jd
Principal Investigator, PI	Dr Stefano Marchesi
Abstract	The X-ray spectral analysis of Compton thick (CT-) active galactic nuclei (AGN)represents a fundamental step to understand the physics of the obscuringmaterial surrounding accreting supermassive black holes. We propose to targetwith a combined NuSTAR/XMM-Newton observation two candidate CT-AGN selected fromthe BAT 100-month volume-limited (z<0.03) sample. Thanks to the excellent countstatistics, we will be able to constrain several spectral parameters (e.g.,relative importance of the scattered component versus the direct one, geometryof the obscuring torus, equivalent width of the Iron emission line). Thisanalysis will refine our knowledge of the selection function of CT-AGN,therefore helping us in determine the true intrinsic fraction of CT-AGN and their contribution to the CXB.
Publications	Compton-thick AGNs in the NuSTAR Era. II. A Deep NuSTAR and XMM-Newton View of the Candidate Compton-thick AGN in NGC 1358 \|Zhao, X., Marchesi, S., et al. \| ApJ \| 870-60 \| 2019 \| 2019ApJ...870...60Z \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...870...60Z Compton-thick AGN in the NuSTAR Era. IV. A Deep NuSTAR and XMM-Newton View of the Candidate Compton-thick AGN in ESO 116-G018 \|Zhao, X., Marchesi, S., \| ApJ \| 871-182 \| 2019 \| 2019ApJ...871..182Z \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...871..182Z Compton-thick AGNs in the NuSTAR Era. III. A Systematic Study of the Torus Covering Factor \|Marchesi, S., Ajello, M., et al. \| ApJ \| 872-8 \| 2019 \| 2019ApJ...872....8M \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...872....8M 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 Compton-thick AGN in the NuSTAR Era. VIII. A joint NuSTAR-XMM-Newton Monitoring of the Changing-look Compton-thick AGN NGC 1358 \|Marchesi, S., Zhao, X., et al. \| ApJ \| 935-114 \| 2022 \| 2022ApJ...935..114M \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...935..114M 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	2017-08-01T16:47:54Z/2017-11-02T11:37:22Z
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	2018-11-21T23:00:00Z
Keywords	"NuSTAR", "equivalent width", "spectral parameters", "fundamental step", ".", "XMM-Newton", "xmm newton", "scattered component", "obscuring torus", "count statistics", "candidate ct agn", "xray spectral analysis", "XMM", "ct agn", "03 sample", "obscuring material", "selection function", "compton thick agn", "iron emission line", "combined nustar", " relative importance"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Stefano Marchesi, 2018, 'COMPTON THICK AGN: THE PHYSICS BEHIND THE OBSCURATION', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-4gxa6jd