A dataset provided by the European Space Agency

Name: MEASURING THE AGN FEEDBACK IN 1H 0419-577
Published: 2011-06-24T00:00:00Z

Proposal ID	060472
Title	MEASURING THE AGN FEEDBACK IN 1H 0419-577
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604720301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604720401
DOI	https://doi.org/10.5270/esa-s9x0oob
Principal Investigator, PI	Dr Elisa Costantini
Abstract	We propose a 160 ks XMM-Newton observation of 1H 0419-577 that will be executednear-simultaneously with an already approved HST-COS observation. We will studythe connection between the X-ray and UV absorber, mapping the ionizationstructure, kinematic behavior and elemental abundances. Finally we will quantifythe AGN feedback by directly measuring the metal enrichment by C, N, O, and Feand the kinetic luminosity of the outflow.
Publications	X-ray variability of 104 active galactic nuclei. XMM-Newton power-spectrum density profiles \|Gonzalez-Martin O. Vaughan S. \| A&A \| 544-80 \| 2012 \| 2012A&A...544A..80G \| http://ui.adsabs.harvard.edu/#abs/2012A&A...544A..80G Simultaneous XMM-Newton and HST-COS observation of 1H0419-577. The absorbing and emitting ionized gas \|Di Gesu L. Costantini E. et al. \| A&A \| 556-94 \| 2013 \| 2013A&A...556A..94D \| http://ui.adsabs.harvard.edu/#abs/2013A&A...556A..94D Variable X-ray reflection from 1H 0419-577 \|Pal Main Dewangan Gulab C. \| MNRAS \| 435-1287 \| 2013 \| 2013MNRAS.435.1287P \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.435.1287P Simultaneous XMM-Newton and HST-COS observation of 1H 0419-577. II. Broadband spectral modeling of a variable Seyfert galaxy \|Di Gesu L. Costantini E. et al. \| A&A \| 563-95 \| 2014 \| 2014A&A...563A..95D \| http://ui.adsabs.harvard.edu/#abs/2014A&A...563A..95D 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 A hard X-ray view of the soft excess in AGN \|Boissay Rozenn Ricci Claudio \| A&A \| 588-70 \| 2016 \| 2016A&A...588A..70B \| http://ui.adsabs.harvard.edu/#abs/2016A&A...588A..70B The Rotation of the Hot Gas around the Milky Way \|Hodges-Kluck Edmund J. Miller Matthew J. \| ApJ \| 822-21 \| 2016 \| 2016ApJ...822...21H \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...822...21H 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 Testing warm Comptonization models for the origin of the soft X-ray excess in AGNs \|Petrucci P.-O. Ursini F. et al. \| A&A \| 611-59 \| 2018 \| 2018A&A...611A..59P \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..59P 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 A relativistic disc reflection model for 1H0419-577: Multi-epoch spectral analysis with XMM-Newton and NuSTAR \|Jiang Jiachen Walton Dominic J. et al. \| MNRAS \| 483-2958 \| 2019 \| 2019MNRAS.483.2958J \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483.2958J 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 Estimating the size of X-ray lamppost coronae in active galactic nuclei \|Ursini F. Dovu010diak M. et al. \| A&A \| 644-132 \| 2020 \| 2020A&A...644A.132U \| http://ui.adsabs.harvard.edu/#abs/2020A&A...644A.132U 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 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 Survey of Bare Active Galactic Nuclei in the Local Universe (z < 0.2). I. On the Origin of Soft Excess \|Nandi Prantik Chatterjee Arka et al. \| ApJS \| 269-15 \| 2023 \| 2023ApJS..269...15N \| http://ui.adsabs.harvard.edu/#abs/2023ApJS..269...15N 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 Unveiling energy pathways in AGN accretion flows with the warm corona model for the soft excess \|Ballantyne D. R. Sudhakar V. et al. \| MNRAS \| 530-1603 \| 2024 \| 2024MNRAS.530.1603B \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.530.1603B 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	2010-05-28T19:41:28Z/2010-05-31T12:40:04Z
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	2011-06-24T00:00:00Z
Last Update	2025-01-27
Keywords	"ionization structure", "uv absorber", "kinetic luminosity", "XMM-Newton", "metal enrichment", "1h 0419 577", "XMM", "elemental abundance", "160 xmm newton", "agn feedback", "approved hst cos", "HST"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Elisa Costantini, 2011, 'MEASURING THE AGN FEEDBACK IN 1H 0419-577', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-s9x0oob