A dataset provided by the European Space Agency

Name: Tracking Down the Ionized Outflow of NGC 7469
Published: 2017-01-15T23:00:00Z

Proposal ID	076035
Title	Tracking Down the Ionized Outflow of NGC 7469
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0760350201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0760350301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0760350401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0760350501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0760350601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0760350701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0760350801
DOI	https://doi.org/10.5270/esa-heqsogn
Principal Investigator, PI	Prof Ehud Behar
Abstract	Using a multiwavelength campaign on NGC 7469, led by XMM-Newton, HST, Swift,NuSTAR, and optical, we propose to achieve new physical insights into theenigmatic AGN winds, by obtaining the deepest ever RGS spectrum of this highly-accreting source. It will allow us to determine the accurate ionisation andchemical structure of the wind. Using EPIC and RGS, we will measure the responseof the outflow to continuum variations, which combined with HST/COS data willunambiguously determine the location, and abundances of the outflow components.Our team pioneered this approach, and applied it successfully (14 refereedpapers) to Mrk 509 that featured only a multi-year response. The uniqueproperties of NGC 7469 make it the ideal candidate to respond on shorter, better-monitored time scales.
Publications	Multi-wavelength campaign on NGC 7469. I. The rich 640 ks RGS spectrum \|Behar, Ehud, Peretz, Uria, et al. \| A&A \| 601-17 \| 2017 \| 2017A&A...601A..17B \| http://ui.adsabs.harvard.edu/#abs/2017A&A...601A..17B Multi-wavelength campaign on NGC 7469. II. Column densities and variability in the X-ray spectrum \|Peretz, U., Behar, E., et al. \| A&A \| 609-35 \| 2018 \| 2018A&A...609A..35P \| http://ui.adsabs.harvard.edu/#abs/2018A&A...609A..35P Multi-wavelength campaign on NCG 7469. IV. The broad-band X-ray spectrum \|Middei, R., Bianchi, S., et al. \| A&A \| 615-163 \| 2018 \| 2018A&A...615A.163M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...615A.163M 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 Application of Clumpy Torus Model to Broadband X-Ray Spectra of Two Seyfert 1 Galaxies: IC 4329A and NGC 7469 \|Ogawa, Shoji, Ueda, Yoshihiro, et al. \| ApJ \| 875-115 \| 2019 \| 2019ApJ...875..115O \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...875..115O The soft X-ray excess: NLS1s versus BLS1s \|Gliozzi, Mario, Williams, James K., \| MNRAS \| 491-532 \| 2020 \| 2020MNRAS.491..532G \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.491..532G Simultaneous Millimetre-wave and X-ray monitoring of the Seyfert galaxy NGC 7469 \|Behar, Ehud, Kaspi, Shai, et al. \| MNRAS \| 491-3523 \| 2020 \| 2020MNRAS.491.3523B \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.491.3523B Multi-wavelength campaign on NGC 7469. VI. Photoionisation modelling of the emission line regions and the warm absorber \|Grafton-Waters, S., Branduardi-Raymont, G., et al. \| A&A \| 633-62 \| 2020 \| 2020A&A...633A..62G \| http://ui.adsabs.harvard.edu/#abs/2020A&A...633A..62G Multi-wavelength campaign on NGC 7469. V. Analysis of the HST/COS observations: Super solar metallicity, distance, and trough variation models \|Arav, N., Xu, X., et al. \| A&A \| 633-61 \| 2020 \| 2020A&A...633A..61A \| http://ui.adsabs.harvard.edu/#abs/2020A&A...633A..61A Systematic Study of AGN Clumpy Tori with Broadband X-Ray Spectroscopy: Updated Unified Picture of AGN Structure \|Ogawa, Shoji, Ueda, Yoshihiro, et al. \| ApJ \| 906-84 \| 2021 \| 2021ApJ...906...84O \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...906...84O 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 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 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 X-Ray Coronal Properties of Swift/BAT-selected Seyfert 1 Active Galactic Nuclei \|Kamraj, Nikita, Brightman, Murray, et al. \| ApJ \| 927-42 \| 2022 \| 2022ApJ...927...42K \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...927...42K Localizing narrow Fe K\\u03b1 emission within bright AGN \|Andonie, Carolina, Bauer, Franz E., et al. \| A&A \| 664-46 \| 2022 \| 2022A&A...664A..46A \| http://ui.adsabs.harvard.edu/#abs/2022A&A...664A..46A 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 Hard X-Ray to Radio Multiwavelength SED Analysis of Local U/LIRGs in the GOALS Sample with a Self-consistent AGN Model including a Polar-dust Component \|Yamada, Satoshi, Ueda, Yoshihiro, et al. \| ApJS \| 265-37 \| 2023 \| 2023ApJS..265...37Y \| http://ui.adsabs.harvard.edu/#abs/2023ApJS..265...37Y 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	2015-06-12T13:36:49Z/2015-12-30T00:54:09Z
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	2017-01-15T23:00:00Z
Keywords	"NuSTAR", "outflow components", "XMM-Newton", "cos data", "xmm newton", "accreting source", "physical insights", "ngc 7469", "monitored time scales", "ionized outflow", "mrk 509", "ideal candidate", "XMM", "multiwavelength campaign", "team pioneered", "rgs spectrum", "continuum variations", "EPIC", "chemical structure", "NGC 7469", "refereed papers", "enigmatic agn winds", "HST"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Ehud Behar, 2017, 'Tracking Down the Ionized Outflow of NGC 7469', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-heqsogn