A dataset provided by the European Space Agency

Name: LMC X-4
Published: 2016-12-12T23:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	077118
Title	LMC X-4
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0771180101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0771180201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0771180301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0771180401
DOI	https://doi.org/10.5270/esa-yomfp1r
Principal Investigator, PI	Dr Ryan Hickox
Abstract	DDT 4 observations of LMC X-4 NuSTAR/XMM-Newton coordinated
Publications	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 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 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 Modeling the Precession of the Warped Inner Accretion Disk in the Pulsars LMC X-4 and SMC X-1 with NuSTAR and XMM-Newton \|Brumback McKinley C. Hickox Ryan C. et al. \| ApJ \| 888-125 \| 2020 \| 2020ApJ...888..125B \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...888..125B 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 Common patterns in pulse profiles of high-mass X-ray binaries \|Alonso-Hernu00e1ndez J. Fu00fcrst F. et al. \| A&A \| 662-62 \| 2022 \| 2022A&A...662A..62A \| http://ui.adsabs.harvard.edu/#abs/2022A&A...662A..62A 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	2015-10-30T02:34:15Z/2015-11-27T14:55:21Z
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	2016-12-12T23:00:00Z
Last Update	2026-07-09
Keywords	"XMM-Newton", "lmc x", "NuSTAR", "XMM", "xmm newton coordinated"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Ryan Hickox, 2016, 'LMC X-4', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-yomfp1r
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.