A dataset provided by the European Space Agency

Name: The soft X-ray component and the hard continuum curvature in black hole binaries
Published: 2015-10-03T22:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	074432
Title	The soft X-ray component and the hard continuum curvature in black hole binaries
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744320201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744320301
DOI	https://doi.org/10.5270/esa-8906mgb
Principal Investigator, PI	Dr Mari Kolehmainen
Abstract	We propose a 40ksec joint XMM-Newton/NuSTAR observation of the black hole binarySwift J1753.5-0127 in its persistent faint low/hard state. This will constrainthe radial stratification of the corona and the spectral curvature of thelow/hard state continuum in the unprecedented 0.7-70keV band. This will thengive the most unambigious measure of the strength of the soft X-ray componentand resolve some of the controversies over the accretion geometry. Theobservation will also help with ongoing calibration/cross- calibration effortsfor both satellites. This observation is not time critical, and will be feasiblewhen it best suits the satellites schedules. An ongoing AMI LA radio monitoringprogramme of Swift J1753.5-0127 will be adapted to coincide with this XMM-Newton/NuSTAR observation.
Publications	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 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 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 Search for Young Stellar Objects within 4XMM-DR13 Using CatBoost and SPE \|Ma Xiangyao Zhang Yanxia et al. \| AJ \| 168-210 \| 2024 \| 2024AJ....168..210M \| http://ui.adsabs.harvard.edu/#abs/2024AJ....168..210M New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2014-09-13T17:41:04Z/2014-09-14T09:48:20Z
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	2015-10-03T22:00:00Z
Last Update	2026-07-09
Keywords	"70kev band", "XMM-Newton", "J1753.5", "blackhole binary", "swift j1753", "hard continuum curvature", "NuSTAR", "XMM", "radial stratification", "spectral curvature", "soft xray component", "ami la radio", "persistent faint low", "cross calibration efforts", "accretion geometry", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Mari Kolehmainen, 2015, 'The soft X-ray component and the hard continuum curvature in black hole binaries', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-8906mgb
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.