A dataset provided by the European Space Agency

Name: Investigating the disc-jet connection in the gamma-ray NLSy1 1H 0323+342
Published: 2016-09-14T22:00:00Z

Proposal ID	076467
Title	Investigating the disc-jet connection in the gamma-ray NLSy1 1H 0323+342
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0764670101
DOI	https://doi.org/10.5270/esa-t9gmh9n
Principal Investigator, PI	Dr Filippo DAmmando
Abstract	The discovery of variable gamma-ray emission from narrow-line Seyfert 1s posesintriguing questions about the formation of relativistic jets, the mechanisms ofhigh-energy production, and the jet-disc connection. We propose a 70 ksecXMM-Newton observation of the gamma-ray NLSy1 1H 0323+342 that will give us thepossibility to investigate the nature of the soft excess and the presence of theIron emission line, inferring important information about the BH spin and theregion of accretion disc responsible for the X-ray emission. Thanks to XMM andFermi-LAT we will also be able to build a detailed SED and study the relationbetween the accretion and jet power in 1H 0323+342, providing for the first timea comprehensive picture of the disc-jet connection in gamma-ray NLSy1.
Publications	The relativistic jet of the gamma-ray emitting narrow-line Seyfert 1 galaxy 1H 0323+342 \|Kynoch Daniel Landt Hermine et al. \| MNRAS \| 475-404 \| 2018 \| 2018MNRAS.475..404K \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.475..404K Independent Estimation of Black Hole Mass for the gamma-ray-detected Archetypal Narrow-line Seyfert 1 Galaxy 1H 0323+342 from X-Ray Variability \|Pan Hai-Wu Yuan Weimin et al. \| ApJ \| 866-69 \| 2018 \| 2018ApJ...866...69P \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...866...69P General Physical Properties of Gamma-Ray-emitting Narrow-line Seyfert 1 Galaxies \|Paliya Vaidehi S. Parker M. L. et al. \| ApJ \| 872-169 \| 2019 \| 2019ApJ...872..169P \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...872..169P Relation between winds and jets in radio-loud AGN \|Mehdipour Missagh Costantini Elisa \| A&A \| 625-25 \| 2019 \| 2019A&A...625A..25M \| http://ui.adsabs.harvard.edu/#abs/2019A&A...625A..25M The origin of X-ray emission in the gamma-ray emitting narrow-line Seyfert 1 1H 0323+342 \|Mundo Sergio A. Kara Erin et al. \| MNRAS \| 496-2922 \| 2020 \| 2020MNRAS.496.2922M \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.496.2922M 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 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	2015-08-23T11:33:40Z/2015-08-24T10:02:00Z
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	2016-09-14T22:00:00Z
Last Update	2025-01-27
Keywords	"disc jet connection", "iron emission line", "jet power", "1h 0323", "relativistic jets", "fermi lat", "xmm newton", "XMM-Newton", "jet disc connection", "energy production", "xray emission", "soft excess", "comprehensive picture", "XMM", "bh spin", "gamma ray nlsy1", "accretion disc"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Filippo D'Ammando, 2016, 'Investigating the disc-jet connection in the gamma-ray NLSy1 1H 0323+342', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-t9gmh9n