A dataset provided by the European Space Agency

Name: PSD BREAK, JET SCALE, AND BLACK-HOLE MASS OF THE FR II RADIO GALAXY 3C 111
Published: 2010-03-11T00:00:00Z

Proposal ID	055218
Title	PSD BREAK, JET SCALE, AND BLACK-HOLE MASS OF THE FR II RADIO GALAXY 3C 111
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0552180101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0552180201
DOI	https://doi.org/10.5270/esa-u9uboix
Principal Investigator, PI	Prof ALAN MARSCHER
Abstract	The investigators request a 130 ks stare of 3C 111 in order to measure thehigh-frequency end of the power spectral density (PSD) of the X-ray fluxvariations. Combined with long-term monitoring with RXTE that is sampling theintermediate and low frequencies, the data will define the break in the PSD.This will add an FR II radio galaxy to the relationship between break frequency,black-hole mass, and accretion rate of both AGNs and XRBs. The long-term lightcurves display dips in X-ray flux that precede the appearance of superluminalknots in the radio jet. The lag between the start of an X-ray event and thefirst appearance of a knot in the jet core will determine the length scale ofthe jet, which we can relate to the black holes gravitational radius.
Publications	The high-energy view of the broad-line radio galaxy 3C 111 \|Ballo L. Braito V. et al. \| MNRAS \| 418-2367 \| 2011 \| 2011MNRAS.418.2367B \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.418.2367B 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 Ultrafast outflows in radio-loud active galactic nuclei \|Tombesi F. Tazaki F. et al. \| MNRAS \| 443-2154 \| 2014 \| 2014MNRAS.443.2154T \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.443.2154T 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 Discussing the physical meaning of the absorption feature at 2.1 keV in 4U 1538-52 \|Rodes-Roca J. J. Torrejon J. M. et al. \| AN \| 335-804 \| 2014 \| 2014AN....335..804R \| http://ui.adsabs.harvard.edu/#abs/2014AN....335..804R Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov V. N. \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y Comparison of ejection events in the jet and accretion disc outflows in 3C 111 \|Tombesi F. Sambruna R. M. et al. \| MNRAS \| 424-754 \| 2012 \| 2012MNRAS.424..754T \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.424..754T X-ray spectral parameters for a sample of 95 active galactic nuclei \|Vasylenko A. A. Zhdanov V. I. \| Ap&SS \| 360-71 \| 2015 \| 2015Ap&SS.360...71V \| http://ui.adsabs.harvard.edu/#abs/2015Ap&SS.360...71V 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 comprehensive analysis of the hard X-ray spectra of bright Seyfert galaxies \|Lubinski P. Beckmann V. et al. \| MNRAS \| 458-2454 \| 2016 \| 2016MNRAS.458.2454L \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.458.2454L 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 Excess Galactic Molecular Absorption Toward the Radio Galaxy 3C 111 \|Tombesi F. Reynolds C. S. et al. \| ApJ \| 842-64 \| 2017 \| 2017ApJ...842...64T \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...842...64T The 3CR Chandra Snapshot Survey: Extragalactic Radio Sources with Redshifts between 1 and 1.5 \|Stuardi C. Missaglia V. et al. \| ApJS \| 235-32 \| 2018 \| 2018ApJS..235...32S \| http://ui.adsabs.harvard.edu/#abs/2018ApJS..235...32S 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 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 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	2009-02-15T14:44:57Z/2009-02-17T04:01:23Z
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	2010-03-11T00:00:00Z
Last Update	2025-01-27
Keywords	"low frequencies", "accretion rate", "xray event", "gravitational radius", "radio jet", "break frequency", "psd break", "xray flux", "fr ii radiogalaxy", "length scale", "blackhole mass", "black hole", "jet scale", "xray flux variations", "3c 111", "superluminal knots"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof ALAN MARSCHER, 2010, 'PSD BREAK, JET SCALE, AND BLACK-HOLE MASS OF THE FR II RADIO GALAXY 3C 111', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-u9uboix