A dataset provided by the European Space Agency

Name: X-ray Spectrometry of SN1987A
Published: 2009-02-07T00:00:00Z

Proposal ID	050622
Title	X-ray Spectrometry of SN1987A
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0506220101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0506220201
DOI	https://doi.org/10.5270/esa-mamnqze
Principal Investigator, PI	Dr Frank Haberl
Abstract	The X-ray luminosity of SN1987A rapidly increased over the last four years, suchthat in a single 100 ks XMM-Newton obervation spectra can be taken withexcellent counting statistics up to energies of 10 keV and more. In reference toour accepted 100 ksec AO5 observation another observation virgul1 year later willallow to study the time evolution of the shock conditions and abundance profilesof N, O, Fe and Ne with RGS. At high energies EPIC-pn can help to clarify theextremely low Fe abundance of 0.04, observed so far. Is the Fe completelyswallowed by the central compact object or is the emission from the innersections of the progenitor star still absorbed? Because of the high number ofcounts a sensitive search for pulses from the pulsar limited to high energy photons will be possible.
Publications	Quasi-stellar Object Selection Algorithm Using Time Variability and Machine Learning: Selection of 1620 Quasi-stellar Object Candidates from MACHO Large Magellanic Cloud Database \|Kim, Dae-Won, Protopapas, Pavlos, et al. \| ApJ \| 735-68 \| 2011 \| 2011ApJ...735...68K \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...735...68K A Refined QSO Selection Method Using Diagnostics Tests: 663 QSO Candidates in the Large Magellanic Cloud \|Kim, Dae-Won, Protopapas, Pavlos, et al. \| ApJ \| 747-107 \| 2012 \| 2012ApJ...747..107K \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...747..107K 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 Suzaku Observations of SN 1987A \|Sturm, Richard, Haberl, Frank, et al. \| PASJ \| 61-895 \| 2009 \| 2009PASJ...61..895S \| http://ui.adsabs.harvard.edu/#abs/2009PASJ...61..895S 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 Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter, J. A., Semba, S., \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog \|Lin, Dacheng, Webb, Natalie A., \| ApJ \| 756-27 \| 2012 \| 2012ApJ...756...27L \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...27L 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 The diversity of quasars unified by accretion and orientation \|Shen, Yue, Ho, Luis C., \| Natur \| 513-210 \| 2014 \| 2014Natur.513..210S \| http://ui.adsabs.harvard.edu/#abs/2014Natur.513..210S 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 A New Sample of Obscured AGNs Selected from the XMM-Newton and AKARI Surveys \|Terashima, Yuichi, Hirata, Yoshitaka, et al. \| ApJ \| 814-11 \| 2015 \| 2015ApJ...814...11T \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...814...11T 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 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, 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	2008-01-11T17:50:57Z/2008-01-13T04:14:44Z
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	2009-02-07T00:00:00Z
Keywords	"energy photons", "xray luminosity", "XMM", "abundance profiles", "progenitor star", "x ray spectrometry", "central compact object", "shock conditions", "inner sections", "counting statistics", "fe completely swallowed", "XMM-Newton", "EPIC", "low fe abundance", "sensitive search", "pulsar limited", "time evolution", "energies epic pn"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Frank Haberl, 2009, 'X-ray Spectrometry of SN1987A', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-mamnqze