A dataset provided by the European Space Agency

Name: Phase Resolved High Resolution Spectroscopy of LMC X-4
Published: 2004-10-12T00:00:00Z

Proposal ID	014280
Title	Phase Resolved High Resolution Spectroscopy of LMC X-4
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0142800101
DOI	https://doi.org/10.5270/esa-jo2znw5
Principal Investigator, PI	Dr Konrad Dennerl
Abstract	We propose to utilize the high spectroscopic capabilities of XMM and itsimpressive photon collection power to study the accreting X-ray binarysystem LMC X-4. With its rich variety of phenomena, LMC X-4 offers awealth of information for detailed studies of the accretion process.Phase resolved spectroscopy of emission lines, in particular of the ironline complex, will not only provide information about the ionizationstages, but also on Doppler broadening and Doppler shifts. Such studiesmay be particularly rewarding for LMC X-4, since EXOSAT observationsshowed evidence for relativistic Doppler splitting of the iron emissionline over the 13.5 s pulse period.
Publications	Spectroscopic Signatures of the Superorbital Period in the Neutron Star Binary LMC X-4 \|Neilsen Joseph Lee Julia C. et al. \| ApJ \| 696-182 \| 2009 \| 2009ApJ...696..182N \| http://ui.adsabs.harvard.edu/#abs/2009ApJ...696..182N The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue \|Watson M. G. Schroder A. C. et al. \| A&A \| 493-339 \| 2009 \| 2009A&A...493..339W \| http://ui.adsabs.harvard.edu/#abs/2009A&A...493..339W Quasi-stellar Object Selection Algorithm Using Time Variability and Machine Learning: Selection of 1620 Quasi-stellar Object Candidates from MACHO Large Magellanic Cloud Database \|Kim Dae-Won Protopapas Pavlos et al. \| ApJ \| 735-68 \| 2011 \| 2011ApJ...735...68K \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...735...68K Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras \|Mateos S. Saxton R. D. et al. \| A&A \| 496-879 \| 2009 \| 2009A&A...496..879M \| http://ui.adsabs.harvard.edu/#abs/2009A&A...496..879M A Refined QSO Selection Method Using Diagnostics Tests: 663 QSO Candidates in the Large Magellanic Cloud \|Kim Dae-Won Protopapas Pavlos et al. \| ApJ \| 747-107 \| 2012 \| 2012ApJ...747..107K \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...747..107K 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 An All-Sky Atlas of Radio/X-ray Associations \|Flesch E. \| PASA \| 27-283 \| 2010 \| 2010PASA...27..283F \| http://ui.adsabs.harvard.edu/#abs/2010PASA...27..283F 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 The XMM-Newton serendipitous ultraviolet source survey catalogue \|Page M. J. Brindle C. et al. \| MNRAS \| 426-903 \| 2012 \| 2012MNRAS.426..903P \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.426..903P 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 Sunyaev-Zeldovich 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 Determination of parameters of Long-Term variability of the X-ray pulsar LMC X-4 \|Molkov S. V. Lutovinov A. A. \| AstL \| 41-562 \| 2015 \| 2015AstL...41..562M \| http://ui.adsabs.harvard.edu/#abs/2015AstL...41..562M The population of X-ray supernova remnants in the Large Magellanic Cloud \|Maggi P. Haberl F. et al. \| A&A \| 585-162 \| 2016 \| 2016A&A...585A.162M \| http://ui.adsabs.harvard.edu/#abs/2016A&A...585A.162M 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 Near-periodical spin period evolution in the binary system LMC X-4 \|Molkov S. Lutovinov A. et al. \| MNRAS \| 464-2039 \| 2017 \| 2017MNRAS.464.2039M \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.464.2039M Post-flare formation of the accretion stream and a dip in pulse profiles of LMC X-4 \|Beri Aru Paul Biswajit \| NewA \| 56-94 \| 2017 \| 2017NewA...56...94B \| http://ui.adsabs.harvard.edu/#abs/2017NewA...56...94B Identification of high-mass X-ray binaries selected from XMM-Newton observations of the LMC* \|van Jaarsveld N. Buckley D. A. H. et al. \| MNRAS \| 475-3253 \| 2018 \| 2018MNRAS.475.3253V \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.475.3253V 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 X-Ray Luminosity and Size Relationship of Supernova Remnants in the LMC \|Ou Po-Sheng Chu You-Hua et al. \| ApJ \| 863-137 \| 2018 \| 2018ApJ...863..137O \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...863..137O 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 X-Ray Reprocessing: Through the Eclipse Spectra of High-mass X-Ray Binaries with XMM-Newton \|Aftab Nafisa Paul Biswajit \| ApJS \| 243-29 \| 2019 \| 2019ApJS..243...29A \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..243...29A 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 New optically identified supernova remnants in the Large Magellanic Cloud \|Yew Miranda Filipoviu0107 Miroslav D. et al. \| MNRAS \| 500-2336 \| 2021 \| 2021MNRAS.500.2336Y \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.500.2336Y 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 Discovery of quasi-periodic oscillations in the persistent X-ray emission of accreting binary X-ray pulsar LMC X-4 \|Rikame Ketan Paul Biswajit et al. \| MNRAS \| 512-4792 \| 2022 \| 2022MNRAS.512.4792R \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.512.4792R A comprehensive study of orbital evolution of LMC X-4: existence of a second derivative of the orbital period \|Jain Chetana Sharma Rahul \| MNRAS \| 529-4056 \| 2024 \| 2024MNRAS.529.4056J \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.529.4056J 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2003-09-09T10:11:34Z/2003-09-10T17:45:47Z
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	2004-10-12T00:00:00Z
Last Update	2025-01-27
Keywords	"emission lines", "resolution spectroscopy", "lmc x", "accretion process", "iron emission line", "iron line complex", "doppler broadening", "pulse period", "relativistic doppler splitting", "phase resolved spectroscopy", "XMM", "phase resolved", "ionization stages", "doppler shifts"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Konrad Dennerl, 2004, 'Phase Resolved High Resolution Spectroscopy of LMC X-4', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-jo2znw5