A dataset provided by the European Space Agency

Name: The first experiment of accretion disc tomography in AGNs
Published: 2014-02-28T00:00:00Z

Proposal ID	069284
Title	The first experiment of accretion disc tomography in AGNs
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0692840201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0692840301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0692840401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0692840501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0692840601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0692840701
DOI	https://doi.org/10.5270/esa-yagp2dx
Principal Investigator, PI	Dr Guido Risaliti
Abstract	We propose four one-orbit observations of the AGN in NGCvirgul1365, with the main aimof measuring the spectral variations during an eclipse. This source showedextraordinary variability in the past observations, indicating a highprobability of catching an eclipse by a Compton-thick cloud in the proposedobservation time. The differences in the shape of the iron broad emission lineat different phases of the eclipse would be a decisive proof of the relativisticeffects on this line due to the strong gravity and fast orbital motion of theinner part of the accretion disc. In addition to this unique experiment, thespectral complexity of NGCvirgul1365 (with the highest S/N detection of ironabsorption lines in AGNs) makes it the ideal target for a deep legacy.. observation.
Publications	A rapidly spinning supermassive black hole at the centre of NGC 1365 \|Risaliti, G., Harrison, F. A., et al. \| Natur \| 494-449 \| 2013 \| 2013Natur.494..449R \| http://ui.adsabs.harvard.edu/#abs/2013Natur.494..449R PCA of PCA: principal component analysis of partial covering absorption in NGC 1365 \|Parker, M. L., Walton, D. J., et al. \| MNRAS \| 441-1817 \| 2014 \| 2014MNRAS.441.1817P \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.441.1817P NuSTAR and XMM-NEWTON Observations of NGC 1365: Extreme Absorption Variability and a Constant Inner Accretion Disk \|Walton, D. J., Risaliti, G., et al. \| ApJ \| 788-76 \| 2014 \| 2014ApJ...788...76W \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...788...76W NGC 1365: A Low Column Density State Unveiling a Low Ionization Disk Wind \|Braito, V., Reeves, J. N., et al. \| ApJ \| 795-87 \| 2014 \| 2014ApJ...795...87B \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...795...87B Iron K and Compton hump reverberation in SWIFT J2127.4+5654 and NGC 1365 revealed by NuSTAR and XMM-Newton \|Kara, E., Zoghbi, A., et al. \| MNRAS \| 446-737 \| 2015 \| 2015MNRAS.446..737K \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.446..737K The Multi-layer Variable Absorbers in NGC 1365 Revealed by XMM-Newton and NuSTAR \|Rivers, E., Risaliti, G., et al. \| ApJ \| 804-107 \| 2015 \| 2015ApJ...804..107R \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...804..107R Non-detection of X-ray emission from sterile neutrinos in stacked galaxy spectra \|Anderson, Michael E., Churazov, Eugene, \| MNRAS \| 452-3905 \| 2015 \| 2015MNRAS.452.3905A \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.452.3905A X-ray spectral parameters for a sample of 95 active galactic nuclei \|Vasylenko, A. A., Zhdanov, V. I., \| Ap&SS \| 360-71 \| 2015 \| 2015Ap&SS.360...71V \| http://ui.adsabs.harvard.edu/#abs/2015Ap&SS.360...71V The Chandra/HETG view of NGC 1365 in a Compton-thick state \|Nardini, E., Gofford, J., et al. \| MNRAS \| 453-2558 \| 2015 \| 2015MNRAS.453.2558N \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.453.2558N Absorption from a multi-layer circumnuclear medium and reflection from the accretion disc in NGC 1365 \|Risaliti, G., \| AN \| 337-529 \| 2016 \| 2016AN....337..529R \| http://ui.adsabs.harvard.edu/#abs/2016AN....337..529R 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 X-ray narrow emission lines from the nuclear region of NGC 1365 \|Whewell, M., Branduardi-Raymont, G., \| A&A \| 595-85 \| 2016 \| 2016A&A...595A..85W \| http://ui.adsabs.harvard.edu/#abs/2016A&A...595A..85W X-ray variability of Seyfert 1.8/1.9 galaxies \|Hernandez-Garcia, L., Masegosa, J., et al. \| A&A \| 602-65 \| 2017 \| 2017A&A...602A..65H \| http://ui.adsabs.harvard.edu/#abs/2017A&A...602A..65H 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 hunt for pulsating ultraluminous X-ray sources \|Song, X., Walton, D. J., et al. \| MNRAS \| 491-1260 \| 2020 \| 2020MNRAS.491.1260S \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.491.1260S 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 spectral evolution in an X-ray changing-look AGN NGC 1365 with variable column density \|Liu, Hao, Wu, Qing-Wen, et al. \| RAA \| 21-199 \| 2021 \| 2021RAA....21..199L \| http://ui.adsabs.harvard.edu/#abs/2021RAA....21..199L Comprehensive Broadband X-Ray and Multiwavelength Study of Active Galactic Nuclei in 57 Local Luminous and Ultraluminous Infrared Galaxies Observed with NuSTAR and/or Swift/BAT \|Yamada, Satoshi, Ueda, Yoshihiro, et al. \| ApJS \| 257-61 \| 2021 \| 2021ApJS..257...61Y \| http://ui.adsabs.harvard.edu/#abs/2021ApJS..257...61Y Variable mass accretion and failed wind explain changing-look phenomena in NGC 1365 \|Mondal, S., Adhikari, T. P., et al. \| A&A \| 662-77 \| 2022 \| 2022A&A...662A..77M \| http://ui.adsabs.harvard.edu/#abs/2022A&A...662A..77M Exploring the Link between the X-Ray Power Spectra and Energy Spectra of Active Galactic Nuclei \|Yang, Haonan, Jin, Chichuan, \| ApJ \| 936-36 \| 2022 \| 2022ApJ...936...36Y \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...936...36Y X-ray timing and spectral analysis of reverberating active galactic nuclei \|Hancock, S., Young, A. J., \| MNRAS \| 514-5403 \| 2022 \| 2022MNRAS.514.5403H \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.514.5403H A Systematic Study of the Short-term X-Ray Variability of Seyfert Galaxies. I. Diversity of the X-Ray rms Spectra \|Hu, Jingwei, Jin, Chichuan, et al. \| ApJ \| 936-105 \| 2022 \| 2022ApJ...936..105H \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...936..105H Dynamical Response of Solar Wind Charge Exchange Soft X-Ray Emission in Earth.s Magnetosphere to the Solar Wind Proton Flux \|Zhang, Yingjie, Sun, Tianran, et al. \| ApJ \| 948-69 \| 2023 \| 2023ApJ...948...69Z \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...948...69Z Testing Physical Scenarios for the Reflection Features of Type-1 AGNs using XMM-Newton and NuSTAR Simultaneous Observations \|Victoria-Ceballos, C\\u00e9sar Ivan, Gonz\\u00e1lez-Mart\\u00edn, Omaira, et al. \| ApJ \| 954-96 \| 2023 \| 2023ApJ...954...96V \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...954...96V Investigating scaling relations in X-ray reverberating AGN using symbolic regression \|Thongkonsing, P., Chainakun, P., et al. \| MNRAS \| 527-1950 \| 2024 \| 2024MNRAS.527.1950T \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.527.1950T 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	2012-07-25T23:29:12Z/2013-02-14T00:22:55Z
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	2014-02-28T00:00:00Z
Keywords	"NGC", "relativistic effects", "accretion disc tomography", "decisive proof", "accretion disc", "extraordinary variability", "deep ``", "compton thick cloud", "spectral complexity", "fast orbital motion", "agns makes", "spectral variations", "ideal target", "iron absorption lines"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Guido Risaliti, 2014, 'The first experiment of accretion disc tomography in AGNs', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-yagp2dx