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-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 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, Filipovi\\u0107, 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
Keywords	"resolution spectroscopy", "doppler broadening", "phase resolved", "iron emission line", "XMM", "phase resolved spectroscopy", "relativistic doppler splitting", "emission lines", "pulse period", "ionization stages", "accretion process", "lmc x", "iron line complex", "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