A dataset provided by the European Space Agency

Name: A Short Look at a Black Hole Transient in Outburst
Published: 2011-05-05T00:00:00Z

Proposal ID	065311
Title	A Short Look at a Black Hole Transient in Outburst
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653110101
DOI	https://doi.org/10.5270/esa-0ouqxq1
Principal Investigator, PI	Dr Jon Miller
Abstract	Recent observations of stellar-mass black holes have revealed evidence of blackhole spin, disk winds, and aspects of how accretion flows vary with the massaccretion rate. We propose to build on these successes with a single 40 ksec(total) observation of a black hole transient in outburst. Though modest, thisobservation will achieve the sensitivity required to place strong constraints onthe nature of the inner disk, and it will help to reveal the nature ofrelationship between disk winds and relativistic jets. We will support thisexposure with a combination of X-ray, optical/IR, and radio observations.
Publications	Multistate observations of the Galactic black hole XTE J1752-223: evidence for an intermediate black hole spin \|Reis R. C. Miller J. M. et al. \| MNRAS \| 410-2497 \| 2011 \| 2011MNRAS.410.2497R \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.410.2497R Multiwavelength Observations of the Black Hole Transient XTE J1752-223 during Its 2010 Outburst Decay \|Chun Y. Y. Dincer T. et al. \| ApJ \| 770-10 \| 2013 \| 2013ApJ...770...10C \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...770...10C 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 Revealing the broad iron Kalpha line in Cygnus X-1 through simultaneous XMM-Newton RXTE and INTEGRAL observations \|Duro Refiz Dauser Thomas et al. \| A&A \| 589-14 \| 2016 \| 2016A&A...589A..14D \| http://ui.adsabs.harvard.edu/#abs/2016A&A...589A..14D 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 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 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 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	2010-04-06T22:28:54Z/2010-04-07T10:07:31Z
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	2011-05-05T00:00:00Z
Last Update	2025-01-27
Keywords	"disk winds", "relativistic jets", "mass accretion rate", "inner disk", "blackhole spin", "accretion flows vary", "blackhole transient", "stellar mass blackhole", "short look"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Jon Miller, 2011, 'A Short Look at a Black Hole Transient in Outburst', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-0ouqxq1