A dataset provided by the European Space Agency

Name: Measuring the disc-jet correlation in SWIFT J1753.5-0127
Published: 2013-09-28T00:00:00Z

Proposal ID	069174
Title	Measuring the disc-jet correlation in SWIFT J1753.5-0127
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0691740201
DOI	https://doi.org/10.5270/esa-rzjoi9y
Principal Investigator, PI	Dr Phil Uttley
Abstract	Simultaneous observations of hard state LMXBs with XMM-Newton and the ISAACinfrared camera on the VLT can reveal the direct connection between accretiondisc variability and variations from the jet. A recent triggered observation ofGX 339-4 revealed the first such correlation and showed, surprisingly, that thedisc is better correlated with the jet IR emission than the power-law is,suggesting that the disc plays a key role in powering the jet. Here we requestan XMM-Newton open time observation (30 ksec exposure) simultaneous withVLT-ISAAC (3 hours) observations of the persistent. LMXB SWIFTvirgulJ1753.5-0127(with a supporting optical observation to be proposed for separately), todetermine whether this exciting result can be applied more generally.
Publications	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 Tracing the Reverberation Lag in the Hard State of Black Hole X-Ray Binaries \|De Marco, B., Ponti, G., et al. \| ApJ \| 814-50 \| 2015 \| 2015ApJ...814...50D \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...814...50D Energy dependence of the band-limited noise in black hole X-ray binaries* \|Stiele, H., Yu, W., \| MNRAS \| 452-3666 \| 2015 \| 2015MNRAS.452.3666S \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.452.3666S Modelling the effect of absorption from the interstellar medium on transient black hole X-ray binaries \|Eckersall, A. J., Vaughan, S., \| MNRAS \| 471-1468 \| 2017 \| 2017MNRAS.471.1468E \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.471.1468E Energy-dependent timing studies of the low-hard state of black hole X-ray binaries with XMM-Newton \|Stiele, Holger, Kong, Albert K. H., \| AN \| 340-314 \| 2019 \| 2019AN....340..314S \| http://ui.adsabs.harvard.edu/#abs/2019AN....340..314S 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
Instrument	EPN, OM, RGS1, RGS2
Temporal Coverage	2012-09-10T17:14:35Z/2012-09-11T04:22:46Z
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	2013-09-28T00:00:00Z
Keywords	"jet ir emission", "accretion disc variability", "XMM", "xmm newton", "vlt isaac", "J1753.5", "disc jet correlation", "disc plays", "supporting optical", "power law", "lmxb swift", "swift j1753", "key role", "XMM-Newton", "gx 339", "isaac infrared camera"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Phil Uttley, 2013, 'Measuring the disc-jet correlation in SWIFT J1753.5-0127', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-rzjoi9y