A dataset provided by the European Space Agency

Name: XMM-Newton Constraints on the AGN Receding Torus Model
Published: 2011-05-05T00:00:00Z

Proposal ID	060643
Title	XMM-Newton Constraints on the AGN Receding Torus Model
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0606430101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0606430201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0606430301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0606430401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0606430501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0606430701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0606430801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0606431101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0606431201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0606431301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0606431401 ...
DOI	https://doi.org/10.5270/esa-8j0w1tt
Principal Investigator, PI	Dr Franz Bauer
Abstract	Recent optical and mid-IR constraints suggest that the putative torussurrounding Active Galactic Nuclei (AGN) may recede with increasing AGN power.Such a result, if true, has important ramifications on AGN unification and theevolution of supermassive black holes (SMBHs). Surprisingly, the bulk of thehigh-z QSOs used to establish this result lack X-ray constraints. We thereforepropose XMM-Newton observations for this otherwise robustly-studied sample toaddress several remaining questions. The resulting X-ray constraints will becompared to existing OIII and 6um AGN continuum luminosities to yield the mostrobust constraints on potential luminosity dependencies to date.
Publications	Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov, V. N., \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y XMM-Newton publication statistics \|Ness, J.-U., Parmar, A. N., et al. \| AN \| 335-210 \| 2014 \| 2014AN....335..210N \| http://ui.adsabs.harvard.edu/#abs/2014AN....335..210N The Tight Relation between X-Ray and Ultraviolet Luminosity of Quasars \|Lusso, E., Risaliti, G., \| ApJ \| 819-154 \| 2016 \| 2016ApJ...819..154L \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...819..154L Spectral clustering for optical confirmation and redshift estimation of X-ray selected galaxy cluster candidates in the SDSS Stripe 82 \|Mahmoud, E., Takey, A., \| A&C \| 16-174 \| 2016 \| 2016A&C....16..174M \| http://ui.adsabs.harvard.edu/#abs/2016A&C....16..174M Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function \|Vagnetti, F., Middei, R., et al. \| A&A \| 593-55 \| 2016 \| 2016A&A...593A..55V \| http://ui.adsabs.harvard.edu/#abs/2016A&A...593A..55V The 3XMM/SDSS Stripe 82 Galaxy Cluster Survey. I. Cluster catalogue and discovery of two merging cluster candidates \|Takey, A., Durret, F., et al. \| A&A \| 594-32 \| 2016 \| 2016A&A...594A..32T \| http://ui.adsabs.harvard.edu/#abs/2016A&A...594A..32T The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch, Eric W., \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton \|Svoboda, J., Guainazzi, M., \| A&A \| 603-127 \| 2017 \| 2017A&A...603A.127S \| http://ui.adsabs.harvard.edu/#abs/2017A&A...603A.127S The 3XMM/SDSS Stripe 82 Galaxy Cluster Survey - II. X-ray and optical properties of the cluster sample \|Takey, Ali, Durret, Florence, et al. \| MNRAS \| 486-4863 \| 2019 \| 2019MNRAS.486.4863T \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.486.4863T X-ray properties of high-richness CAMIRA clusters in the Hyper Suprime-Cam Subaru Strategic Program field \|Ota, Naomi, Mitsuishi, Ikuyuki, et al. \| PASJ \| 72-1 \| 2020 \| 2020PASJ...72....1O \| http://ui.adsabs.harvard.edu/#abs/2020PASJ...72....1O 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 A Luminous X-Ray Transient in SDSS J143359.16+400636.0: A Likely Tidal Disruption Event \|Brightman, Murray, Ward, Charlotte, et al. \| ApJ \| 909-102 \| 2021 \| 2021ApJ...909..102B \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...909..102B 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 X-ray emission from a rapidly accreting narrow-line Seyfert 1 galaxy at z = 6.56 \|Wolf, J., Nandra, K., et al. \| A&A \| 669-127 \| 2023 \| 2023A&A...669A.127W \| http://ui.adsabs.harvard.edu/#abs/2023A&A...669A.127W 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	2009-11-01T21:38:10Z/2010-04-04T16:17:33Z
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	2011-05-05T00:00:00Z
Keywords	"supermassive blackhole smbhs", "agn unification", "agn power", "XMM", "z qsos", "mid ir constraints", "xray constraints", "xmm newton constraints", "robust constraints", "potential luminosity", "XMM-Newton", "otherwise robustly", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Franz Bauer, 2011, 'XMM-Newton Constraints on the AGN Receding Torus Model', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-8j0w1tt