A dataset provided by the European Space Agency

Name: Deep X-ray view of the bare nucleus Seyfert Ark120: unveiling the core of AGN
Published: 2015-04-29T22:00:00Z

Proposal ID	072160
Title	Deep X-ray view of the bare nucleus Seyfert Ark120: unveiling the core of AGN
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721600201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721600301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721600401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721600501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721600601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721600701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721600801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721600901
DOI	https://doi.org/10.5270/esa-v5urfbr
Principal Investigator, PI	Dr Delphine Porquet
Abstract	truncated We propose here a deep XMM-Newton observation (4 x 120 ks) of Ark120-- and a joint 120ks Chandra/HETG observation to measure the narrow FeK linecore -- to establish the origin of the soft excess (Comptonization or blurredreflection), its accretion disk properties and its black hole spin. If the softexcess originates from blurred reflection off an ionized accretion disk, we willbe able to clearly detect and resolve, for the first time unambiguously in aBLS1 AGN, broad soft X-ray lines (e.g., OVII, OVIII and FeL). It will be thefirst very high S/N X-ray observation of a bare AGN.
Publications	A Deep X-Ray View of the Bare AGN Ark 120. I. Revealing the Soft X-Ray Line Emission \|Reeves, J. N., Porquet, D., et al. \| ApJ \| 828-98 \| 2016 \| 2016ApJ...828...98R \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...828...98R 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 A Deep X-Ray View of the Bare AGN Ark 120. II. Evidence for Fe K Emission Transients \|Nardini, E., Porquet, D., et al. \| ApJ \| 832-45 \| 2016 \| 2016ApJ...832...45N \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...832...45N Energy-dependent variability of the bare Seyfert 1 galaxy Ark 120 \|Mallick, Labani, Dewangan, Gulab C., et al. \| MNRAS \| 472-174 \| 2017 \| 2017MNRAS.472..174M \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.472..174M A deep X-ray view of the bare AGN Ark 120. III. X-ray timing analysis and multiwavelength variability \|Lobban, A. P., Porquet, D., et al. \| MNRAS \| 474-3237 \| 2018 \| 2018MNRAS.474.3237L \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.474.3237L A deep X-ray view of the bare AGN Ark 120. IV. XMM-Newton and NuSTAR spectra dominated by two temperature (warm, hot) Comptonization processes \|Porquet, D., Reeves, J. N., et al. \| A&A \| 609-42 \| 2018 \| 2018A&A...609A..42P \| http://ui.adsabs.harvard.edu/#abs/2018A&A...609A..42P Are narrow-line Seyfert 1 galaxies highly accreting low-MBH AGNs? \|Williams, James K., Gliozzi, Mario, \| MNRAS \| 480-96 \| 2018 \| 2018MNRAS.480...96W \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.480...96W Multicomponent power-density spectra of Kepler AGNs, an instrumental artefact or a physical origin? \|Dobrotka, A., Bezak, P., et al. \| MNRAS \| 483-38 \| 2019 \| 2019MNRAS.483...38D \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483...38D A deep X-ray view of the bare AGN Ark 120. VI. Geometry of the hot corona from spectroscopic and polarization signatures \|Marinucci, A., Porquet, D., et al. \| A&A \| 623-12 \| 2019 \| 2019A&A...623A..12M \| http://ui.adsabs.harvard.edu/#abs/2019A&A...623A..12M A deep X-ray view of the bare AGN Ark 120. V. Spin determination from disc-Comptonisation efficiency method \|Porquet, D., Done, C., et al. \| A&A \| 623-11 \| 2019 \| 2019A&A...623A..11P \| http://ui.adsabs.harvard.edu/#abs/2019A&A...623A..11P High Density Reflection Spectroscopy - II. The density of the inner black hole accretion disc in AGN \|Jiang, Jiachen, Fabian, Andrew C., et al. \| MNRAS \| 489-3436 \| 2019 \| 2019MNRAS.489.3436J \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.489.3436J On the Observational Difference between the Accretion Disk-Corona Connections among Super- and Sub-Eddington Accreting Active Galactic Nuclei \|Liu, Hezhen, Luo, B., et al. \| ApJ \| 910-103 \| 2021 \| 2021ApJ...910..103L \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...910..103L 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 Nitrogen X-ray absorption in the local ISM \|Gatuzz, Efrain, Garc\\u00eda, Javier A., \| MNRAS \| 504-4460 \| 2021 \| 2021MNRAS.504.4460G \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.504.4460G Long-term X-ray observations of seyfert 1 galaxy ark 120: on the origin of soft-excess \|Nandi, Prantik, Chatterjee, Arka, et al. \| MNRAS \| 506-3111 \| 2021 \| 2021MNRAS.506.3111N \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.506.3111N Fundamental X-ray corona parameters of Swift/BAT AGN \|Hinkle, Jason T., Mushotzky, Richard, \| MNRAS \| 506-4960 \| 2021 \| 2021MNRAS.506.4960H \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.506.4960H 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 Origins of the UV/X-ray relation in Arakelian 120 \|Mahmoud, R. D., Done, C., et al. \| MNRAS \| 521-3585 \| 2023 \| 2023MNRAS.521.3585M \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.521.3585M Soft excess in AGN with relativistic X\\u2011ray reflection \|Ezhikode, Savithri H., Shyam Prakash V., P., et al. \| AN \| 344-20230042 \| 2023 \| 2023AN....34430042E \| http://ui.adsabs.harvard.edu/#abs/2023AN....34430042E 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 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 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	2014-03-18T06:55:49Z/2014-03-25T21:01:33Z
Version	PPS_NOT_AVAILABLE
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	2015-04-29T22:00:00Z
Keywords	"blurred reflection", "accretion disk properties", "deep xmm newton", "bls1 agn", "XMM", " ovii", "bare agn", "120 chandra", "time unambiguously", "soft excess comptonization", "XMM-Newton", "ionized accretion disk", "blackhole spin", "x 120", ".", "deep xray", "soft excess originates"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Delphine Porquet, 2015, 'Deep X-ray view of the bare nucleus Seyfert Ark120: unveiling the core of AGN', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-v5urfbr