A dataset provided by the European Space Agency

Name: X-ray Spectrometry of SN1987A
Published: 2017-11-23T23:00:00Z

Proposal ID	078325
Title	X-ray Spectrometry of SN1987A
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783250201
DOI	https://doi.org/10.5270/esa-wp7q612
Principal Investigator, PI	Dr Frank Haberl
Abstract	Between 2007 and 2014, 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, which levelled off in 2014. To further monitor theevolution of the X-ray flux and look for the expected turn-over we propose tocontinue our monitoring. This will allow us to further study the time evolutionof the shock conditions and abundance profiles. At high energies EPIC-pn canhelp to clarify the extremely low observed Fe abundance by following theevolution 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 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 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 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 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	2016-11-02T06:32:33Z/2016-11-03T03:29:13Z
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	2017-11-23T23:00:00Z
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, 2017, 'X-ray Spectrometry of SN1987A', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-wp7q612