A dataset provided by the European Space Agency

Name: Identifying & understanding the X-ray binary populations of the SMC
Published: 2015-01-10T23:00:00Z

Proposal ID	070058
Title	Identifying & understanding the X-ray binary populations of the SMC
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0700580101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0700580401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0700580601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0700580701
DOI	https://doi.org/10.5270/esa-epabw2v
Principal Investigator, PI	Prof Malcolm Coe
Abstract	The LMC & SMC represent an exceptional opportunity to study the evolution ofX-ray binaries under very different conditions to those in the Milky Way.They are close enough for the individual sources to be detected, identii??ed &studied, whilst presenting diverse environments in terms of metallicity andtidal effects. In this proposal we request regular monitoring of the SMC with Integral to locate new transient pulsar systems and to continue exploring the a??100 known & suspected HMXB systems. Precise source location will be achievedwith XMM. The source locations are critical to unlock the full potential science of the HMXB systems and it enables us to explore stellar and binary evolution in different chemical and tidal environments.
Publications	SXP 5.05 = IGR J00569-7226: using X-rays to explore the structure of a Be stars circumstellar disc \|Coe M. J. Bartlett E. S. et al. \| MNRAS \| 447-2387 \| 2015 \| 2015MNRAS.447.2387C \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.447.2387C Spectroscopic characterization of X-ray emitting young stars associated with the Sh 2-296 nebula \|Fernandes B. Gregorio-Hetem J. et al. \| MNRAS \| 448-119 \| 2015 \| 2015MNRAS.448..119F \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.448..119F High-mass X-ray binaries in the Small Magellanic Cloud \|Haberl F. Sturm R. \| A&A \| 586-81 \| 2016 \| 2016A&A...586A..81H \| http://ui.adsabs.harvard.edu/#abs/2016A&A...586A..81H The Chandra ACIS Timing Survey Project: glimpsing a sample of faint X-ray pulsators \|Israel G. L. Esposito P. et al. \| MNRAS \| 462-4371 \| 2016 \| 2016MNRAS.462.4371I \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.462.4371I 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 SXP 7.92: a recently rediscovered Be/X-ray binary in the Small Magellanic Cloud viewed edge on \|Bartlett E. S. Coe M. J. et al. \| MNRAS \| 466-4659 \| 2017 \| 2017MNRAS.466.4659B \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.466.4659B A Comprehensive Library of X-Ray Pulsars in the Small Magellanic Cloud: Time Evolution of Their Luminosities and Spin Periods \|Yang J. Laycock S. G. T. et al. \| ApJ \| 839-119 \| 2017 \| 2017ApJ...839..119Y \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...839..119Y Deep Chandra Survey of the Small Magellanic Cloud. II. Timing Analysis of X-Ray Pulsars \|Hong JaeSub Antoniou Vallia et al. \| ApJ \| 847-26 \| 2017 \| 2017ApJ...847...26H \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...847...26H Identification of AGN in the XMM-Newton X-ray survey of the SMC \|Maitra Chandreyee Haberl Frank et al. \| A&A \| 622-29 \| 2019 \| 2019A&A...622A..29M \| http://ui.adsabs.harvard.edu/#abs/2019A&A...622A..29M The supernova remnant population of the Small Magellanic Cloud \|Maggi Pierre Filipoviu0107 Miroslav D. et al. \| A&A \| 631-127 \| 2019 \| 2019A&A...631A.127M \| http://ui.adsabs.harvard.edu/#abs/2019A&A...631A.127M 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 Spitzer and Herschel studies of dust in supernova remnants in the Small Magellanic Cloud \|Matsuura Mikako Ayley Victoria et al. \| MNRAS \| 513-1154 \| 2022 \| 2022MNRAS.513.1154M \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.513.1154M 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 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	2013-11-01T10:21:54Z/2013-12-26T19:05:10Z
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	2015-01-10T23:00:00Z
Last Update	2025-08-04
Keywords	"XMM", "binary evolution", "suspected hmxb systems", "xray binary populations", "source locations", "diverse environments", "tidal environments", "transient pulsar systems", "hmxb systems", "potential science", "tidal effects", "precise source location", "explore stellar", "individual sources", "xray binary"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Malcolm Coe, 2015, 'Identifying & understanding the X-ray binary populations of the SMC', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-epabw2v