A dataset provided by the European Space Agency

Name: X-ray Spectrometry of SN1987A
Published: 2014-01-15T00:00:00Z

Proposal ID	069051
Title	X-ray Spectrometry of SN1987A
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690510101
DOI	https://doi.org/10.5270/esa-1bzb5bt
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. At high energiesEPIC-pn can help to clarify the extremely low observed Fe abundance by followingthe evolution of the detected Fe-K line. Is most of the Fe swallowed by thecentral compact object or is the emission from the inner sections of the progenitor star still absorbed?
Publications	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 Supernova 1987A: a Template to Link Supernovae to Their Remnants \|Orlando, S., Miceli, M., et al. \| ApJ \| 810-168 \| 2015 \| 2015ApJ...810..168O \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...810..168O 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, Filipovi\\u0107, 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 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	2012-12-11T03:34:12Z/2012-12-11T22:59:28Z
Version	14.21_20150826_1500
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	2014-01-15T00:00:00Z
Keywords	"XMM", "abundance profiles", "yearly xmm newton", "progenitor star", "x ray spectrometry", "central compact object", "numerous emission lines", "ofsupernova1987a yields epic", "shock conditions", "inner sections", "fe abundance", "XMM-Newton", "EPIC", "fe swallowed", "rgs spectra", "time evolution", "xmm newton", "energies epic pn"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Frank Haberl, 2014, 'X-ray Spectrometry of SN1987A', 14.21_20150826_1500, European Space Agency, https://doi.org/10.5270/esa-1bzb5bt