A dataset provided by the European Space Agency

Name: BH spin and Fe K line variability: entering the precision era
Published: 2011-12-22T00:00:00Z

Proposal ID	065545
Title	BH spin and Fe K line variability: entering the precision era
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655450101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655450201
DOI	https://doi.org/10.5270/esa-4fsw8jz
Principal Investigator, PI	Dr Giovanni Miniutti
Abstract	We have observed the INTEGRAL/BAT NLS1 galaxy SWIFT J2127.4+5654 with Suzaku in2007. Our observation revealed the unambigous presence of a broad iron (Fe) linefrom the accretion disc in this very bright source. The Suzaku observationallowed us to measure via Fe line diagnostics a black hole spin a~0.6. However,constraints are not yet very precise and, with the proposed observation, we aimat entering the precision era for BH spin measuremments. Moreover, tentativeline profile was observed during the Suzaku observation. Our proposed 130~ksexposure with XMM-Newton will be used to reveal the line variability and itsresponse (or lack of it) to the continuum variation.
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 The size of the X-ray emitting region in SWIFT J2127.4+5654 via a broad line region cloud X-ray eclipse \|Sanfrutos M. Miniutti G. et al. \| MNRAS \| 436-1588 \| 2013 \| 2013MNRAS.436.1588S \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.436.1588S Search for X-ray occultations in active galactic nuclei \|Torricelli-Ciamponi G. Pietrini P. et al. \| MNRAS \| 442-2116 \| 2014 \| 2014MNRAS.442.2116T \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.442.2116T 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 A search for X-ray reprocessing echoes in the power spectral density functions of AGN \|Emmanoulopoulos D. Papadakis I. E. et al. \| MNRAS \| 461-1642 \| 2016 \| 2016MNRAS.461.1642E \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.461.1642E 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 X-ray occultations in active galactic nuclei: distribution in size of orbiting clouds and total mass content in the cloud ensemble \|Pietrini P. Torricelli-Ciamponi G. \| A&A \| 628-26 \| 2019 \| 2019A&A...628A..26P \| http://ui.adsabs.harvard.edu/#abs/2019A&A...628A..26P High Density Reflection Spectroscopy - II. The density of the inner black hole accretion disc in AGN \|Jiang Jiachen Fabian Andrew C. et al. \| MNRAS \| 489-3436 \| 2019 \| 2019MNRAS.489.3436J \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.489.3436J 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 Hard Look at Relativistic Reverberation in MCG-5-23-16 and SWIFT J2127.4+5654: Testing the Lamppost Model \|Zoghbi A. Miller J. M. \| ApJ \| 912-42 \| 2021 \| 2021ApJ...912...42Z \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...912...42Z 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 value-added catalogue of ASAS-SN eclipsing binaries: parameters of 30 000 detached systems \|Rowan D. M. Jayasinghe T. et al. \| MNRAS \| 517-2190 \| 2022 \| 2022MNRAS.517.2190R \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.517.2190R 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	2010-11-29T17:30:23Z/2010-12-01T07:23:08Z
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	2011-12-22T00:00:00Z
Last Update	2025-01-27
Keywords	"continuum variation", "precision era", "unambigous presence", "J2127.4", "xmm newton", "tentative line profile", "XMM-Newton", "line variability", "bright source", "blackhole spin", "bh spin", "XMM", "bh spin measuremments", "accretion disc"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Giovanni Miniutti, 2011, 'BH spin and Fe K line variability: entering the precision era', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-4fsw8jz