A dataset provided by the European Space Agency

Name: Unveiling the underlying nature of the new class of HMXBs discovered by INTEGRAL
Published: 2008-04-14T00:00:00Z

Proposal ID	040614
Title	Unveiling the underlying nature of the new class of HMXBs discovered by INTEGRAL
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0406140101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0406140201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0406140301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0406140401
DOI	https://doi.org/10.5270/esa-a6cykew
Principal Investigator, PI	Prof Anthony Dean
Abstract	Of the 200+ galactic sources observed by INTEGRAL a consistent fraction of thepoint sources have not been associated with previously indentified objects.Follow up studies have identified that a significant number of these sources arehighly obscured, HMXBs with a neutron star companion. Understanding the detailedmechanics of these systems and their place in the general picture of binary starevolution are the dual objectives of this proposal. We request observing time toexploit the powerful spectroscopic, imaging and timing capabilitie of XMM tofind counterparts for 7 unidentified, persistent INTEGRAL sources discovered bythe IBIS/ISGRI instrument, which are clustered in the Crux spiral arm tangentand are HMXB candidates. Thus identify the nature of the underlying system.
Publications	The Two Integral X-Ray Transients IGR J17091-3624 and IGR J17098-3628: A Multiwavelength Long-Term Campaign \|Capitanio, F., Giroletti, M., et al. \| ApJ \| 690-1621 \| 2009 \| 2009ApJ...690.1621C \| http://ui.adsabs.harvard.edu/#abs/2009ApJ...690.1621C The supergiant fast X-ray transient IGRJ18483-0311 in quiescence: XMM-Newton, Swift and Chandra observations \|Giunta, A., Bozzo, E., et al. \| MNRAS \| 399-744 \| 2009 \| 2009MNRAS.399..744G \| http://ui.adsabs.harvard.edu/#abs/2009MNRAS.399..744G XMM-Newton and INTEGRAL study of the SFXT IGR J18483-0311 in quiescence: hint of a cyclotron emission feature? \|Sguera, V., Ducci, L., et al. \| MNRAS \| 402-49 \| 2010 \| 2010MNRAS.402L..49S \| http://ui.adsabs.harvard.edu/#abs/2010MNRAS.402L..49S The enigmatic black hole candidate and X-ray transient IGR J17091-3624 in its quiescent state as seen with XMM-Newton \|Wijnands, R., Yang, Y. J., \| MNRAS \| 422-91 \| 2012 \| 2012MNRAS.422L..91W \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.422L..91W The XMM Cluster Survey: optical analysis methodology and the first data release \|Mehrtens, Nicola, Romer, A. Kathy, et al. \| MNRAS \| 423-1024 \| 2012 \| 2012MNRAS.423.1024M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M The Galactic plane at faint X-ray fluxes - I. Properties and characteristics of the X-ray source population \|Warwick, R. S., Perez-Ramirez, D., \| MNRAS \| 413-595 \| 2011 \| 2011MNRAS.413..595W \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.413..595W The XMM Cluster Survey: X-ray analysis methodology \|Lloyd-Davies, E. J., Romer, A. Kathy, et al. \| MNRAS \| 418-14 \| 2011 \| 2011MNRAS.418...14L \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.418...14L Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter, J. A., Semba, S., \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C Chandra Observations of Five INTEGRAL Sources: New X-Ray Positions for IGR J16393-4643 and IGR J17091-3624 \|Bodaghee, A., Rahoui, F., et al. \| ApJ \| 751-113 \| 2012 \| 2012ApJ...751..113B \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...751..113B Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog \|Lin, Dacheng, Webb, Natalie A., \| ApJ \| 756-27 \| 2012 \| 2012ApJ...756...27L \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...27L Spectral and temporal properties of the supergiant fast X-ray transient IGR J18483-0311 observed by INTEGRAL \|Ducci, L., Doroshenko, V., et al. \| A&A \| 559-135 \| 2013 \| 2013A&A...559A.135D \| http://ui.adsabs.harvard.edu/#abs/2013A&A...559A.135D The Galactic plane at faint X-ray fluxes - II. Stacked X-ray spectra of a sample of serendipitous XMM-Newton sources \|Warwick, R. S., Byckling, K., \| MNRAS \| 438-2967 \| 2014 \| 2014MNRAS.438.2967W \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.438.2967W Automatic Classification of Time-variable X-Ray Sources \|Lo, Kitty K., Farrell, Sean, et al. \| ApJ \| 786-20 \| 2014 \| 2014ApJ...786...20L \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...786...20L The diversity of quasars unified by accretion and orientation \|Shen, Yue, Ho, Luis C., \| Natur \| 513-210 \| 2014 \| 2014Natur.513..210S \| http://ui.adsabs.harvard.edu/#abs/2014Natur.513..210S 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 An XMM-Newton view of FeKalpha in high-mass X-ray binaries \|Gimenez-Garcia, A., Torrejon, J. M., et al. \| A&A \| 576-108 \| 2015 \| 2015A&A...576A.108G \| http://ui.adsabs.harvard.edu/#abs/2015A&A...576A.108G Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters \|Xiao, Weike, Chen, Chen, et al. \| MNRAS \| 432-41 \| 2013 \| 2013MNRAS.432L..41X \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X 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 Anisotropy of the galaxy cluster X-ray luminosity-temperature relation \|Migkas, Konstantinos, Reiprich, Thomas H., \| A&A \| 611-50 \| 2018 \| 2018A&A...611A..50M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..50M The XMM Cluster Survey: Present status and latest results \|Viana, P. T. P., Mehrtens, N., et al. \| AN \| 334-462 \| 2013 \| 2013AN....334..462V \| http://ui.adsabs.harvard.edu/#abs/2013AN....334..462V Testing emergent gravity on galaxy cluster scales \|Tamosiunas, Andrius, Bacon, David, et al. \| JCAP \| 5-53 \| 2019 \| 2019JCAP...05..053T \| http://ui.adsabs.harvard.edu/#abs/2019JCAP...05..053T Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline \|Hollowood, Devon L., Jeltema, Tesla, et al. \| ApJS \| 244-22 \| 2019 \| 2019ApJS..244...22H \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters \|Palmese, A., Annis, J., et al. \| MNRAS \| 493-4591 \| 2020 \| 2020MNRAS.493.4591P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P 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 From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez, Antonio C., \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R 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	2006-06-24T07:18:22Z/2007-02-19T19:16:15Z
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	2008-04-14T00:00:00Z
Keywords	"binary star evolution", "isgri instrument", "neutron star companion", "XMM", "persistent integral sources", "dual objectives", "galactic sources", "indentified objects", "hmxb candidates", "powerful spectroscopic"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Anthony Dean, 2008, 'Unveiling the underlying nature of the new class of HMXBs discovered by INTEGRAL', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-a6cykew