A dataset provided by the European Space Agency

Name: Bridging the X-ray Variability Properties of Supermassive and Galactic Black H
Published: 2015-02-05T23:00:00Z

Proposal ID	072310
Title	Bridging the X-ray Variability Properties of Supermassive and Galactic Black H
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723100301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723100401
DOI	https://doi.org/10.5270/esa-ce4wkf7
Principal Investigator, PI	Dr Brandon Kelly
Abstract	We propose to obtain new XMM light curves of 5 AGN with reverberation-basedblack hole mass from the Lick AGN Monitoring Project (LAMP) to investigate howtheir variability properties scale with black hole mass and Eddington ratio.These 5 sources are among the AGN with the smallest measured black hole masses(M_BH = 1E6-1E7 M_Sun), making them an important bridge between the variabilityproperties of supermassive and stellar mass black holes. Moreover, we will usethe XMM observations to calibrate X-ray variability as a mass estimator at lowmasses for AGN, which can be used to search for the seeds of supermassive blackholes in nearby bulge less dwarf galaxies.
Publications	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 The broad-band spectrum of the narrow-line Seyfert 1 NGC 4748: from UV to hard X-ray \|Vasylenko A. A. \| Ap&SS \| 363-228 \| 2018 \| 2018Ap&SS.363..228V \| http://ui.adsabs.harvard.edu/#abs/2018Ap&SS.363..228V 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 Narrow-Line SY1 NGC 4748 in X-Rays: Detailed Case-Study \|Vasylenko A. Fedorova E. \| ARep \| 64-384 \| 2020 \| 2020ARep...64..384V \| http://ui.adsabs.harvard.edu/#abs/2020ARep...64..384V On the Observational Difference between the Accretion Disk-Corona Connections among Super- and Sub-Eddington Accreting Active Galactic Nuclei \|Liu Hezhen Luo B. et al. \| ApJ \| 910-103 \| 2021 \| 2021ApJ...910..103L \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...910..103L Hard X-Ray Emission Associated with White Dwarfs. IV. Signs of Accretion from Substellar Companions \|Chu You-Hua Toalu00e1 Jesu00fas A. et al. \| ApJ \| 910-119 \| 2021 \| 2021ApJ...910..119C \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...910..119C 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 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	2013-12-09T09:40:31Z/2014-01-15T01:53:03Z
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	2015-02-05T23:00:00Z
Last Update	2025-01-27
Keywords	"variability properties", "calibrate xray variability", "dwarf galaxy", "xray variability properties", "low masses", "galactic black", "lick agn", "1e6 1e7 m_sun", "eddington ratio", "project lamp", "blackhole masses m_bh", "mass estimator", "blackhole mass", "nearby bulge", "XMM", "xmm light curves", "variability properties scale", "supermassive blackhole"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Brandon Kelly, 2015, 'Bridging the X-ray Variability Properties of Supermassive and Galactic Black H', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ce4wkf7