A dataset provided by the European Space Agency

Name: X-ray Spectrometry of SN1987A
Published: 2012-01-22T00:00:00Z

Proposal ID	065042
Title	X-ray Spectrometry of SN1987A
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0650420101
DOI	https://doi.org/10.5270/esa-rpdzxn1
Principal Investigator, PI	Dr Frank Haberl
Abstract	Since Jan. 2007, our yearly XMM-Newton monitoring of SN 1987A yields EPIC andRGS spectra of unprecedented quality. The fluxes and broadening of the numerousemission lines provide information on the evolution of the X-ray emitting plas-ma and its dynamics. The soft X-ray light curve shows a significant flatteningafter 2006. To further monitor the turn-over we propose to continue our XMM-Newton monitoring of SN 1987A. This will allow us to further study the timeevolution of the shock conditions and abundance profiles of, e.g., N, O, Fe, Ne.At high energies EPIC-pn can help to clarify the low Fe abundance observed sofar. Is the Fe completely swallowed by the central compact object or is theemission from the inner sections of the progenitor star still absorbed?
Publications	Evolution and Hydrodynamics of the Very Broad X-Ray Line Emission in SN 1987A \|Dewey D. Dwarkadas V. V. et al. \| ApJ \| 752-103 \| 2012 \| 2012ApJ...752..103D \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...752..103D XMM-Newton observations of SNR 1987A. II. The still increasing X-ray light curve and the properties of Fe K lines \|Maggi P. Haberl F. et al. \| A&A \| 548-3 \| 2012 \| 2012A&A...548L...3M \| http://ui.adsabs.harvard.edu/#abs/2012A&A...548L...3M 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 XMM-Newton study of 30 Doradus C and a newly identified MCSNR J0536-6913 in the Large Magellanic Cloud* \|Kavanagh P. J. Sasaki M. et al. \| A&A \| 573-73 \| 2015 \| 2015A&A...573A..73K \| http://ui.adsabs.harvard.edu/#abs/2015A&A...573A..73K 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 A Spatially Resolved Study of X-Ray Properties in Superbubble 30 Dor C with XMM-Newton \|Babazaki Yasunori Mitsuishi Ikuyuki et al. \| ApJ \| 864-12 \| 2018 \| 2018ApJ...864...12B \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...864...12B 3D MHD modeling of the expanding remnant of SN 1987A. Role of magnetic field and non-thermal radio emission \|Orlando S. Miceli M. et al. \| A&A \| 622-73 \| 2019 \| 2019A&A...622A..73O \| http://ui.adsabs.harvard.edu/#abs/2019A&A...622A..73O 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 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	2010-12-12T02:02:34Z/2010-12-12T20:21:10Z
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	2012-01-22T00:00:00Z
Last Update	2025-01-27
Keywords	"time evolution", "EPIC", "progenitor star", "ofsupernova1987a yields epic", "yearly xmm newton", "xmm newton", "x ray spectrometry", "XMM-Newton", "numerous emission lines", "low fe abundance", "abundance profiles", "rgs spectra", "inner sections", "energies epic pn", "XMM", "shock conditions", "central compact object", "fe completely swallowed"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Frank Haberl, 2012, 'X-ray Spectrometry of SN1987A', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-rpdzxn1