A dataset provided by the European Space Agency

Name: The hard state of a transient black hole: is the accretion disk truncatedquestionMark
Published: 2017-03-29T22:00:00Z

Proposal ID	074396
Title	The hard state of a transient black hole: is the accretion disk truncated?
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743960201
DOI	https://doi.org/10.5270/esa-h2iar0y
Principal Investigator, PI	Prof Fiona Harrison
Abstract	The combination of the fast EPIC-pn modes and broad-band coverage with RXTEproved to be an effective means of exploring accretion in bright Galactic blackholes. XMM and NuSTAR provide an even more powerful combination. We propose tomake one joint 40virgulks observation of a new or known black hole transient during abright, hard outburst phase. The goals of this program are to 1) measure thespin of the black hole via the Fe K-alpha line and broad-band disk reflectionspectrum, 2) test an apparent anti-correlation between winds and jets in softand hard states by making a very sensitive search for winds in a hard,intermediate, or very high state. This observation will be supported by anetwork of ground-based observatories and X-ray monitoring.
Publications	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 Discovering the Mass-Scaled Damping Timescale from Microquasars to Blazars \|Zhang, Haoyang, Yang, Shenbang, \| ApJ \| 967-L18 \| 2024 \| 2024ApJ...967L..18Z \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...967L..18Z 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	2016-03-07T04:04:10Z/2016-03-07T21:19:10Z
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	2017-03-29T22:00:00Z
Keywords	"NuSTAR", "alpha line", "effective means", "XMM", "powerful combination", "broad band coverage", "blackhole via", "hard outburst phase", "apparent anti correlation", "exploring accretion", "EPIC", "blackhole transient", "rxte proved", "sensitive search", "transient black hole"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Fiona Harrison, 2017, 'The hard state of a transient black hole: is the accretion disk truncatedquestionMark', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-h2iar0y