A dataset provided by the European Space Agency

Name: X-ray Spectrometry of SN1987A
Published: 2015-12-23T23:00:00Z

Proposal ID	074379
Title	X-ray Spectrometry of SN1987A
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743790101
DOI	https://doi.org/10.5270/esa-e73ojmj
Principal Investigator, PI	Dr Frank Haberl
Abstract	Between 2007 and 2012, our yearly XMM-Newton monitoring of SN1987A yielded EPICand RGS spectra of unprecedented quality. The fluxes and broadening of thenumerous emission lines provide information on the evolution of the X-rayemitting plasma and its dynamics. The soft X-ray light curve shows a mildflattening after 2006. To further monitor the evolution of the X-ray flux andlook for a possible turn-over we propose to continue our monitoring. This willallow us to further study the time evolution of the shock conditions andabundance profiles. At high energies EPIC-pn can help to clarify the extremelylow observed Fe abundance by following the evolution of the detected Fe-K line.
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 Chandra Observes the End of an Era in SN 1987A \|Frank Kari A. Zhekov Svetozar A. et al. \| ApJ \| 829-40 \| 2016 \| 2016ApJ...829...40F \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829...40F 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 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 Evidence of Particle Acceleration in the Superbubble 30 Doradus C with NuSTAR \|Lopez Laura A. Grefenstette Brian W. et al. \| ApJ \| 893-144 \| 2020 \| 2020ApJ...893..144L \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...893..144L 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 BAT99 126: A multiple Wolf-Rayet system in the Large Magellanic Cloud with a massive near-contact binary \|Janssens S. Shenar T. et al. \| A&A \| 646-33 \| 2021 \| 2021A&A...646A..33J \| http://ui.adsabs.harvard.edu/#abs/2021A&A...646A..33J 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 Post-impact Evolution of the X-Ray-emitting Gas in SNR 1987A as Viewed by XMM-Newton \|Sun Lei Vink Jacco et al. \| ApJ \| 916-41 \| 2021 \| 2021ApJ...916...41S \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...916...41S Thermal Emission and Radioactive Lines but No Pulsar in the Broadband X-Ray Spectrum of Supernova 1987A \|Alp Dennis Larsson Josefin \| ApJ \| 916-76 \| 2021 \| 2021ApJ...916...76A \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...916...76A Associated Molecular and Atomic Clouds with X-Ray Shell of Superbubble 30 Doradus C in the LMC \|Yamane Y. Sano H. et al. \| ApJ \| 918-36 \| 2021 \| 2021ApJ...918...36Y \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...918...36Y SN 1987A: Tracing the flux decline and spectral evolution through a comparison of SRG/eROSITA and XMM-Newton observations \|Maitra C. Haberl F. et al. \| A&A \| 661-30 \| 2022 \| 2022A&A...661A..30M \| http://ui.adsabs.harvard.edu/#abs/2022A&A...661A..30M Additional Evidence for a Pulsar Wind Nebula in the Heart of SN 1987A from Multiepoch X-Ray Data and MHD Modeling \|Greco Emanuele Miceli Marco et al. \| ApJ \| 931-132 \| 2022 \| 2022ApJ...931..132G \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...931..132G An exploration of X-ray Supernova remnants in the Milky Way and nearby galaxies \|Albert Chris Dwarkadas Vikram V. \| MNRAS \| 514-728 \| 2022 \| 2022MNRAS.514..728A \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.514..728A Thermal X-ray emission in the western half of the LMC superbubble 30 Dor C \|Chi Yi-Heng Chen Han-Xiao et al. \| MNRAS \| 530-4219 \| 2024 \| 2024MNRAS.530.4219C \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.530.4219C 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	2014-11-29T04:41:41Z/2014-11-30T03:06:41Z
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	2015-12-23T23:00:00Z
Last Update	2025-01-27
Keywords	"time evolution", "EPIC", "yearly xmm newton", "x ray spectrometry", "XMM-Newton", "numerous emission lines", "xray flux", "rgs spectra", "abundance profiles", "fe abundance", "xray emitting plasma", "XMM", "energies epic pn", "mild flattening", "shock conditions"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Frank Haberl, 2015, 'X-ray Spectrometry of SN1987A', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-e73ojmj