A dataset provided by the European Space Agency

Name: IRAS17020+4544: the first case of a warm absorber in a Radio-Loud NL Seyfert 1
Published: 2015-02-10T23:00:00Z

Proposal ID	072122
Title	IRAS17020+4544: the first case of a warm absorber in a Radio-Loud NL Seyfert 1
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721220101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721220301
DOI	https://doi.org/10.5270/esa-2uzx1ff
Principal Investigator, PI	Dr Anna Lia Longinotti
Abstract	We propose to obtain a deep exposure (150 ks) of the radio-loud NLS1 galaxyIRAS17020+4544. This is a relatively unexplored source that presents peculiarcharacteristics. Archival X-ray data show a multicomponent warm absorber in thesoft X-ray spectrum and spectral complexity in the Fe K band, suggestingabsorption in highly ionized Iron. Recent VLBA observations revealed a compactradio structure and a well defined jet component. Given the known radio andX-ray properties of the source, this target represents one of the best candidatefor: 1) studying the properties of outflowing gas in one of the rare radio loudsources where this phenomenon is detected and 2) studying the effect of ionizedabsorption in the Fe K band.
Publications	X-Ray High-resolution Spectroscopy Reveals Feedback in a Seyfert Galaxy from an Ultra-fast Wind with Complex Ionization and Velocity Structure \|Longinotti A. L. Krongold Y. et al. \| ApJ \| 813-39 \| 2015 \| 2015ApJ...813L..39L \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...813L..39L 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 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 The Evolution of the Warm Absorber Reveals a Shocked Outflow in the Narrow Line Seyfert 1 Galaxy IRAS 17020+4544 \|Sanfrutos Mario Longinotti Anna Lia et al. \| ApJ \| 868-111 \| 2018 \| 2018ApJ...868..111S \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...868..111S Characterizing continuum variability in the radio-loud narrow-line Seyfert 1 galaxy IRAS 17020+4544 \|Gonzalez A. G. Gallo L. C. et al. \| MNRAS \| 496-3708 \| 2020 \| 2020MNRAS.496.3708G \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.496.3708G 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 UV Counterpart of an X-Ray Ultrafast Outflow in IRAS 17020+4544 \|Mehdipour Missagh Kriss Gerard A. et al. \| ApJ \| 930-166 \| 2022 \| 2022ApJ...930..166M \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930..166M 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 NOEMA spatially resolved view of the multiphase outflow in IRAS17020+4544: a shocked wind in action? \|Longinotti Anna Lia Salomu00e9 Q. et al. \| MNRAS \| 521-2134 \| 2023 \| 2023MNRAS.521.2134L \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.521.2134L 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	2014-01-23T10:36:55Z/2014-01-26T09:34:28Z
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	2015-02-10T23:00:00Z
Last Update	2025-01-27
Keywords	"archival xray data", "target represents", "ionized absorption", "soft xray spectrum", "defined jet component", "relatively unexplored source", "multicomponent warm absorber", "warm absorber", "spectral complexity", "xray properties", "outflowing gas", "compact radio structure", "deep exposure", "ionized iron"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Anna Lia Longinotti, 2015, 'IRAS17020+4544: the first case of a warm absorber in a Radio-Loud NL Seyfert 1', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-2uzx1ff