A dataset provided by the European Space Agency

Name: X-ray Spectrometry of SN1987A
Published: 2010-03-07T00:00:00Z

Proposal ID	055635
Title	X-ray Spectrometry of SN1987A
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0556350101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0556350201
DOI	https://doi.org/10.5270/esa-5nlj1ru
Principal Investigator, PI	Dr Frank Haberl
Abstract	From a 100 ks XMM-Newton observation of SN 1987A performed in Jan. 2007 (AO5) weobtained EPIC and RGS spectra of unprecedented quality. The soft X-ray lightcurve shows a significant flattening since the beginning of 2006. To monitorthis turn-over we propose to continue our yearly XMM-Newton observations of SN1987A. Together with our accepted AO6 observation this will allow us to studythe time evolution of the shock conditions and abundance profiles of, e.g., N,O, Fe, Ne (with RGS). At high energies EPIC-pn can help to clarify the extremelylow Fe abundance observed so far. Is the Fe completely swallowed by the centralcompact object or is the emission from the inner sections of the progenitor starstill 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 High resolution X-ray spectroscopy of SN 1987 A: monitoring with XMM-Newton \|Sturm, R., Haberl, F., et al. \| A&A \| 515-5 \| 2010 \| 2010A&A...515A...5S \| http://ui.adsabs.harvard.edu/#abs/2010A&A...515A...5S 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, 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 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	2009-01-30T15:26:00Z/2009-01-31T22:35:34Z
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	2010-03-07T00:00:00Z
Keywords	"ofsupernova1987a performed", "XMM", "abundance profiles", "yearly xmm newton", "progenitor star", "x ray spectrometry", "central compact object", "shock conditions", "inner sections", "2007 ao5", "fe completely swallowed", "XMM-Newton", "EPIC", "low fe abundance", "rgs spectra", "time evolution", "xmm newton", "energies epic pn"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Frank Haberl, 2010, 'X-ray Spectrometry of SN1987A', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-5nlj1ru