A dataset provided by the European Space Agency

Name: Fast multi-wavelength variability from a black hole
Published: 2014-10-16T22:00:00Z

Proposal ID	069234
Title	Fast multi-wavelength variability from a black hole
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0692341201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0692341301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0692341401
DOI	https://doi.org/10.5270/esa-y83kqio
Principal Investigator, PI	Dr Kieran O.Brien
Abstract	Correlated fast multi-wavelength variability is becoming a key tool forstudying the physics of accretion and ejection of relativistic jets. Usingsimultaneous X-ray and near-infrared data we have recently discovered vibrationsfrom a relativistic jet down to 62.5 ms time scale, which allowed us to estimatethe speed and the size of the jet. We have shown that the properties of thejet depend on the spectral state of the black hole. We will monitor the outburstevolution of a black hole transient with XMM, simultaneously with ground-basedoptical and IR facilities, in order to apply the same technique to differentspectral states. We propose to perform 10 short (7 ksec) XMM observations ofan active black hole, in order to cover the different stages of the outburst.
Publications	The Complex Accretion Geometry of GX 339-4 as Seen by NuSTAR and Swift \|Furst, F., Nowak, M. A., et al. \| ApJ \| 808-122 \| 2015 \| 2015ApJ...808..122F \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...808..122F Spectral analysis of the XMM-Newton data of GX 339-4 in the low/hard state: disc truncation and reflection \|Basak, Rupal, Zdziarski, Andrzej A., \| MNRAS \| 458-2199 \| 2016 \| 2016MNRAS.458.2199B \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.458.2199B 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 Evolution of GX 339-4 in the Low-hard State as Seen by NuSTAR and Swift \|Wang-Ji, Jingyi, Garcia, Javier A., et al. \| ApJ \| 855-61 \| 2018 \| 2018ApJ...855...61W \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...855...61W 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 X-Ray AGB Stars in the 4XMM-DR9 Catalog: Further Evidence for Companions \|Ortiz, R., Guerrero, M. A., \| ApJ \| 912-93 \| 2021 \| 2021ApJ...912...93O \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...912...93O High-density Reflection Spectroscopy of Black Hole X-Ray Binaries in the Hard State \|Liu, Honghui, Jiang, Jiachen, et al. \| ApJ \| 951-145 \| 2023 \| 2023ApJ...951..145L \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...951..145L The current state of disk wind observations in BHLMXBs through X-ray absorption lines in the iron band \|Parra, M., Petrucci, P. -O., et al. \| A&A \| 681-49 \| 2024 \| 2024A&A...681A..49P \| http://ui.adsabs.harvard.edu/#abs/2024A&A...681A..49P 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	2013-09-29T22:49:07Z/2013-10-02T00:48:49Z
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	2014-10-16T22:00:00Z
Keywords	"XMM", "outburst evolution", "ms time scale", "key tool", "ir facilities", "black hole", "relativistic jet", "relativistic jets", "jet depend", "active black hole", "blackhole transient", "infrared data"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Kieran O.Brien, 2014, 'Fast multi-wavelength variability from a black hole', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-y83kqio