A dataset provided by the European Space Agency

Name: Exporing the PSD of RX J1140.1+030: an IMBH accreting at super-Eddington rate
Published: 2015-01-20T23:00:00Z

Proposal ID	072484
Title	Exporing the PSD of RX J1140.1+030: an IMBH accreting at super-Eddington rate
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724840101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724840301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724840401
DOI	https://doi.org/10.5270/esa-nrui0gd
Principal Investigator, PI	Dr Chichuan Jin
Abstract	So far there is only one AGN, Ark 564, whose power spectral density (PSD) showsa multi-Lorentzian shape which is similar to that seen in BHBs emitting in thevery high state. Recently we discovered that the PSD of the NLS1 RXJ1140.1+0307, which is claimed to harbor an intermediate mass black hole with asuper-Eddington accretion rate, also appears to have more than one Lorentziancomponent. However, the previous XMM observation is too short to extend the PSDto lower frequency. Therefore we propose a long (120 ks) XMM-Newton observationof RX J1140.1+0307, in order to perform a deep investigation of its PSD, alongwith other variability properties. Because such phenomenon observed in the PSDof AGN are extremely rare, it is important to study the best examples in detail.
Publications	Strong constraints on a super-Eddington accretion flow: XMM-Newton observations of an intermediate-mass black hole \|Jin Chichuan Done Chris \| MNRAS \| 455-691 \| 2016 \| 2016MNRAS.455..691J \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.455..691J XMM-Newton publication statistics \|Ness J.-U. Parmar A. N. et al. \| AN \| 335-210 \| 2014 \| 2014AN....335..210N \| http://ui.adsabs.harvard.edu/#abs/2014AN....335..210N 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 AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton \|Svoboda J. Guainazzi M. \| A&A \| 603-127 \| 2017 \| 2017A&A...603A.127S \| http://ui.adsabs.harvard.edu/#abs/2017A&A...603A.127S A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies \|Ojha Vineet Chand Hum et al. \| ApJ \| 896-95 \| 2020 \| 2020ApJ...896...95O \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...95O Discovery of soft and hard X-ray time lags in low-mass AGNs \|Mallick L. Wilkins D. R. et al. \| MNRAS \| 503-3775 \| 2021 \| 2021MNRAS.503.3775M \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.3775M 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 High-density disc reflection spectroscopy of low-mass active galactic nuclei \|Mallick L. Fabian A. C. et al. \| MNRAS \| 513-4361 \| 2022 \| 2022MNRAS.513.4361M \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.513.4361M 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	2013-12-18T14:03:25Z/2014-01-02T10:09:34Z
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	2015-01-20T23:00:00Z
Keywords	"rx j1140", "lower frequency", "nls1 rx j1140", "XMM", "J1140.1", "120 xmm newton", "lorentzian component", "multi lorentzian shape", "variability properties", "imbh accreting", "bhbs emitting", "ark 564", "XMM-Newton", "deep investigation", "intermediate mass blackhole", "super eddington rate"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Chichuan Jin, 2015, 'Exporing the PSD of RX J1140.1+030: an IMBH accreting at super-Eddington rate', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-nrui0gd