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
License: https://creativecommons.org/licenses/by-nc/3.0/igo

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 SWIFT~J1753.5-0127(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 The accretion discs of transient X-ray binaries \|Eckersall Alexander James \| PhDT \| 0-57 \| 2018 \| 2018PhDT........57E \| http://ui.adsabs.harvard.edu/#abs/2018PhDT........57E Fast X-ray/IR observations of the black hole transient Swift J1753.5u20130127: From an IR lead to a very long jet lag \|Ulgiati A. Vincentelli F. M. et al. \| A&A \| 690-A239 \| 2024 \| 2024A&A...690A.239U \| http://ui.adsabs.harvard.edu/#abs/2024A&A...690A.239U
Instrument	EPN, OM, RGS1, RGS2
Temporal Coverage	2012-09-10T17:14:35Z/2012-09-11T04:22:46Z
Version	21.51_20241115_1113
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
Last Update	2026-07-09
Keywords	"vlt isaac", "jet ir emission", "XMM-Newton", "key role", "J1753.5", "gx 339", "disc plays", "swift j1753", "isaac infrared camera", "XMM", "lmxb swift", "disc jet correlation", "supporting optical", "accretion disc variability", "power law", "xmm newton"
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', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-rzjoi9y
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.