A dataset provided by the European Space Agency

Name: The Unique Case of PKS J1220+0203: a jetted AGN with a broad Iron Line
Published: 2018-06-30T22:00:00Z

Proposal ID	080256
Title	The Unique Case of PKS J1220+0203: a jetted AGN with a broad Iron Line
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0802560101
DOI	https://doi.org/10.5270/esa-jz7w2ey
Principal Investigator, PI	Dr Marco Ajello
Abstract	PKS J1220+0203 is the only AGN with a relativistic jet, whose X-ray spectrum isreflection dominated and boasts a broad Iron line emission with equivalent widthof 1.2 keV. Because of the jet inclination angle and the lack of obscuration, webelieve this emission arises in the inner regions of the accretion disk and itis relativistically blurred. As such it provides a unique opportunity to probethe geometry and state of the accretion flow near the black hole and the blackhole spin. We propose to acquire a high signal-to-noise spectrum with XMM-Newtonand NuSTAR to study the accretion flow and measure the black hole spin in thisvery interesting object.
Publications	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 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	2017-06-07T09:07:19Z/2017-06-08T00:07:19Z
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	2018-06-30T22:00:00Z
Last Update	2025-01-27
Keywords	"inner region", "accretion disk", "jetted agn", "xmm newton", "equivalent width", "XMM-Newton", "blackhole spin", "jet inclination angle", "NuSTAR", "broad iron line", "relativistic jet", "XMM", "xray spectrum", "relativistically blurred", "reflection dominated", "noise spectrum", "accretion flow"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Marco Ajello, 2018, 'The Unique Case of PKS J1220+0203: a jetted AGN with a broad Iron Line', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-jz7w2ey