A dataset provided by the European Space Agency

Name: Mapping the inner accretion flow: dynamic reverberation in IRAS 13224-3809
Published: 2016-08-26T22:00:00Z

Proposal ID	078056
Title	Mapping the inner accretion flow: dynamic reverberation in IRAS 13224-3809
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0780560101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0780561301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0780561401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0780561501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0780561601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0780561701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0780562401
DOI	https://doi.org/10.5270/esa-gfb8qrt
Principal Investigator, PI	Prof Andrew Fabian
Abstract	The Narrow-Line Seyfert 1 galaxy IRAS13224-3809 shows strong iron-K and L broadlines and high-frequency soft X-ray time lags indicating reflection from theinnermost regions about a rapidly spinning black hole. It persistently varieswith high amplitude changes every 2 to 3 days. The peak frequency and energyspectrum of the lags varies with flux, probably due to changes in size of thecorona. We propose a Very Large Programme consisting of a 1.5Ms observation ofthis object, which will enable the full range of flux levels to be studied,yielding a dynamic picture of the changing height and size of the corona andtransforming our understanding of how luminous black hole accretion operates.
Publications	The response of relativistic outflowing gas to the inner accretion disk of a black hole \|Parker, Michael L., Pinto, Ciro, et al. \| Natur \| 543-83 \| 2017 \| 2017Natur.543...83P \| http://ui.adsabs.harvard.edu/#abs/2017Natur.543...83P Revealing the ultrafast outflow in IRAS 13224-3809 through spectral variability \|Parker, M. L., Alston, W. N., et al. \| MNRAS \| 469-1553 \| 2017 \| 2017MNRAS.469.1553P \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.469.1553P Is there a UV/X-ray connection in IRAS 13224-3809? \|Buisson, D. J. K., Lohfink, A. M., et al. \| MNRAS \| 475-2306 \| 2018 \| 2018MNRAS.475.2306B \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.475.2306B Ultrafast outflows disappear in high-radiation fields \|Pinto, C., Alston, W., et al. \| MNRAS \| 476-1021 \| 2018 \| 2018MNRAS.476.1021P \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.476.1021P The 1.5 Ms observing campaign on IRAS 13224-3809 - I. X-ray spectral analysis \|Jiang, J., Parker, M. L., et al. \| MNRAS \| 477-3711 \| 2018 \| 2018MNRAS.477.3711J \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.477.3711J Can the relativistic light-bending model explain X-ray spectral variations of Seyfert galaxies? \|Mizumoto, Misaki, Moriyama, Kotaro, et al. \| PASJ \| 70-42 \| 2018 \| 2018PASJ...70...42M \| http://ui.adsabs.harvard.edu/#abs/2018PASJ...70...42M The Variable Relativistic Outflow of IRAS 13224--3809 \|Chartas, George, Canas, Manuel H., \| ApJ \| 867-103 \| 2018 \| 2018ApJ...867..103C \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...867..103C The remarkable X-ray variability of IRAS 13224-3809 - I. The variability process \|Alston, W. N., Fabian, A. C., et al. \| MNRAS \| 482-2088 \| 2019 \| 2019MNRAS.482.2088A \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.482.2088A Non-stationary variability in accreting compact objects \|Alston, W. N., \| MNRAS \| 485-260 \| 2019 \| 2019MNRAS.485..260A \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.485..260A Modelling X-ray RMS spectra I: intrinsically variable AGNs \|Parker, M. L., Alston, W. N., et al. \| MNRAS \| 492-1363 \| 2020 \| 2020MNRAS.492.1363P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.492.1363P Blueshifted absorption lines from X-ray reflection in IRAS 13224-3809 \|Fabian, A. C., Reynolds, C. S., et al. \| MNRAS \| 493-2518 \| 2020 \| 2020MNRAS.493.2518F \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.2518F A dynamic black hole corona in an active galaxy through X-ray reverberation mapping \|Alston, William N., Fabian, Andrew C., et al. \| NatAs \| 4-597 \| 2020 \| 2020NatAs...4..597A \| http://ui.adsabs.harvard.edu/#abs/2020NatAs...4..597A A combined timing/spectral study of IRAS 13224-3809 using XMM-Newton data \|Caballero-Garc\\u00eda, M. D., Papadakis, I. E., et al. \| MNRAS \| 498-3184 \| 2020 \| 2020MNRAS.498.3184C \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.498.3184C Searching for energy-resolved quasi-periodic oscillations in AGN \|Ashton, Dominic I., Middleton, Matthew J., \| MNRAS \| 501-5478 \| 2021 \| 2021MNRAS.501.5478A \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.501.5478A 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 Spectral-timing of AGN ionized outflows with Athena \|Jur\\u00e1\\u0148ov\\u00e1, A., Costantini, E., \| MNRAS \| 510-4225 \| 2022 \| 2022MNRAS.510.4225J \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.510.4225J Constraining energy-dependent emissivity profiles of AGN inflows \|Ashton, Dominic I., Middleton, Matthew J., \| MNRAS \| 513-5245 \| 2022 \| 2022MNRAS.513.5245A \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.513.5245A XMM-Newton observations of the narrow-line Seyfert 1 galaxy IRAS 13224-3809: X-ray spectral analysis II \|Jiang, Jiachen, Dauser, Thomas, et al. \| MNRAS \| 514-1107 \| 2022 \| 2022MNRAS.514.1107J \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.514.1107J Mapping the X-Ray Corona Evolution of IRAS 13224-3809 with the Power Spectral Density \|Chainakun, Poemwai, Luangtip, Wasuthep, et al. \| ApJ \| 934-166 \| 2022 \| 2022ApJ...934..166C \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...934..166C 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 Extended corona models of X-ray reverberation in the AGN 1H 0707-495 and IRAS 13224-3809 \|Hancock, S., Young, A. J., \| MNRAS \| 520-180 \| 2023 \| 2023MNRAS.520..180H \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.520..180H A novel \\spectral\\u2011ratio model fitting\\ to resolve complicated X\\u2011ray spectral variations in active galactic nuclei \|Midooka, Takuya, Mizumoto, Misaki, \| AN \| 344-20230039 \| 2023 \| 2023AN....34430039M \| http://ui.adsabs.harvard.edu/#abs/2023AN....34430039M Revealing the intrinsic X-ray reverberation lags in IRAS 13224-3809 through the Granger causality test \|Chainakun, P., Nakhonthong, N., et al. \| MNRAS \| 523-111 \| 2023 \| 2023MNRAS.523..111C \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.523..111C Coronal height constraint in IRAS 13224-3809 and 1H 0707-495 by the random forest regressor \|Mankatwit, N., Chainakun, P., et al. \| MNRAS \| 523-4080 \| 2023 \| 2023MNRAS.523.4080M \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.523.4080M Radiatively Driven Clumpy X-Ray Absorbers in the NLS1 Galaxy IRAS 13224-3809 \|Midooka, Takuya, Mizumoto, Misaki, \| ApJ \| 954-47 \| 2023 \| 2023ApJ...954...47M \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...954...47M Applying wavelet analysis to the X-ray light curves of active galactic nuclei and quasi-periodic eruptions \|Ghosh, Akshay, Gallo, L. C., \| MNRAS \| 524-1478 \| 2023 \| 2023MNRAS.524.1478G \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.524.1478G Wavelet spectral timing: X-ray reverberation from a dynamic black hole corona hidden beneath ultrafast outflows \|Wilkins, D. R., \| MNRAS \| 526-3441 \| 2023 \| 2023MNRAS.526.3441W \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.526.3441W 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 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 Tracing the evolving X-ray reverberation lags within an individual AGN light curve \|Nakhonthong, N., Chainakun, P., et al. \| MNRAS \| 530-1894 \| 2024 \| 2024MNRAS.530.1894N \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.530.1894N 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	2016-07-08T19:33:33Z/2016-07-26T09:35:08Z
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	2016-08-26T22:00:00Z
Keywords	"innermost region", "dynamic reverberation", "spinning black hole", "inner accretion flow", "energy spectrum", "dynamic picture", "iras 13224 3809", "changing height", "broad lines", "flux levels", "narrow line seyfert", "programme consisting", "persistently varies", "peak frequency", "galaxy iras13224 3809", "lags varies"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Andrew Fabian, 2016, 'Mapping the inner accretion flow: dynamic reverberation in IRAS 13224-3809', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-gfb8qrt