A dataset provided by the European Space Agency

Name: Spectroscopy of thermal supernova remnants in the Magellanic Clouds SSC_1
Published: 2003-11-14T00:00:00Z

Proposal ID	011113
Title	Spectroscopy of thermal supernova remnants in the Magellanic Clouds SSC_1
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111130101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111130201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111130301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111130401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111130501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111130701
DOI	https://doi.org/10.5270/esa-nmawhut
Principal Investigator, PI	Dr Michael Watson
Abstract	GT-We propose to observe a sample of thermal supernova remnants in the MagellanicClouds, with the RGS (high resolution spectroscopy) and the EPIC (broadband, high sensitivity spectroscopy, spectro-imaging). Our aim is toobserve remnants at a well-known distance in order to test SNR models andqualify statistical studies over larger samples. The XMM RGS offers the opportunity to obtain global spectra at spectral resolution of 100 or so around 1 keV. This is crucial for distinguishing lines in thermal spectra. The XMM EPIC will have the sensitivity to extend the spectral data to high energy and to provide imaging in the lines.
Publications	High mass X-ray binaries in the LMC: Dependence on the stellar population age and the propeller effect \|Shtykovskiy P. Gilfanov M. \| A&A \| 431-597 \| 2005 \| 2005A&A...431..597S \| http://ui.adsabs.harvard.edu/#abs/2005A&A...431..597S Quiet but still bright: XMM-Newton observations of the soft gamma-ray repeater SGR0526-66 \|Tiengo A. Esposito P. et al. \| MNRAS \| 399-74 \| 2009 \| 2009MNRAS.399L..74T \| http://ui.adsabs.harvard.edu/#abs/2009MNRAS.399L..74T The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue \|Watson M. G. Schroder A. C. et al. \| A&A \| 493-339 \| 2009 \| 2009A&A...493..339W \| http://ui.adsabs.harvard.edu/#abs/2009A&A...493..339W 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 Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras \|Mateos S. Saxton R. D. et al. \| A&A \| 496-879 \| 2009 \| 2009A&A...496..879M \| http://ui.adsabs.harvard.edu/#abs/2009A&A...496..879M 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 The XMM Cluster Survey: optical analysis methodology and the first data release \|Mehrtens Nicola Romer A. Kathy et al. \| MNRAS \| 423-1024 \| 2012 \| 2012MNRAS.423.1024M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M XMM-Newton X-ray spectra of the SNR 0509-67.5: data and models \|Kosenko D. Vink J. et al. \| A&A \| 490-223 \| 2008 \| 2008A&A...490..223K \| http://ui.adsabs.harvard.edu/#abs/2008A&A...490..223K The Persistence of Memory or How the X-Ray Spectrum of SNR 0509-67.5 Reveals the Brightness of Its Parent Type Ia Supernova \|Badenes Carles Hughes John P. et al. \| ApJ \| 680-1149 \| 2008 \| 2008ApJ...680.1149B \| http://ui.adsabs.harvard.edu/#abs/2008ApJ...680.1149B Dusty Blast Waves of Two Young Large Magellanic Cloud Supernova Remnants: Constraints on Post-shock Compression \|Williams Brian J. Borkowski Kazimierz J. et al. \| ApJ \| 729-65 \| 2011 \| 2011ApJ...729...65W \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...729...65W An All-Sky Atlas of Radio/X-ray Associations \|Flesch E. \| PASA \| 27-283 \| 2010 \| 2010PASA...27..283F \| http://ui.adsabs.harvard.edu/#abs/2010PASA...27..283F Supernova remnant energetics and magnetars: no evidence in favour of millisecond proto-neutron stars \|Vink Jacco Kuiper Lucien \| MNRAS \| 370-14 \| 2006 \| 2006MNRAS.370L..14V \| http://ui.adsabs.harvard.edu/#abs/2006MNRAS.370L..14V The high resolution X-ray spectrum of SNR 0506-68 using XMM-Newton \|Broersen S. Vink J. et al. \| A&A \| 535-11 \| 2011 \| 2011A&A...535A..11B \| http://ui.adsabs.harvard.edu/#abs/2011A&A...535A..11B The XMM Cluster Survey: X-ray analysis methodology \|Lloyd-Davies E. J. Romer A. Kathy et al. \| MNRAS \| 418-14 \| 2011 \| 2011MNRAS.418...14L \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.418...14L 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 An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities \|Henley David B. Shelton Robin L. \| ApJS \| 202-14 \| 2012 \| 2012ApJS..202...14H \| http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H The XMM-Newton serendipitous ultraviolet source survey catalogue \|Page M. J. Brindle C. et al. \| MNRAS \| 426-903 \| 2012 \| 2012MNRAS.426..903P \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.426..903P Properties of the integrated spectrum of serendipitous 2XMM catalog sources \|Chaudhary P. Brusa M. et al. \| A&A \| 518-58 \| 2010 \| 2010A&A...518A..58C \| http://ui.adsabs.harvard.edu/#abs/2010A&A...518A..58C Rest-frame stacking of 2XMM catalog sources. Properties of the Fe Kalpha line \|Chaudhary P. Brusa M. et al. \| A&A \| 537-6 \| 2012 \| 2012A&A...537A...6C \| http://ui.adsabs.harvard.edu/#abs/2012A&A...537A...6C A systematic cross-search for radio/infrared counterparts of XMM- Newton sources \|Combi J. A. Albacete Colombo J. F. et al. \| Ap&SS \| 331-53 \| 2011 \| 2011Ap&SS.331...53C \| http://ui.adsabs.harvard.edu/#abs/2011Ap&SS.331...53C The 2-8 keV cosmic X-ray background spectrum as observed with XMM-Newton \|De Luca A. Molendi S. \| A&A \| 419-837 \| 2004 \| 2004A&A...419..837D \| http://ui.adsabs.harvard.edu/#abs/2004A&A...419..837D 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 Sunyaev-Zeldovich effect or not? Detecting the main foreground effect of most galaxy clusters \|Xiao Weike Chen Chen et al. \| MNRAS \| 432-41 \| 2013 \| 2013MNRAS.432L..41X \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X Oxygen emission in remnants of thermonuclear supernovae as a probe for their progenitor system \|Kosenko D. Hillebrandt W. et al. \| MNRAS \| 449-1441 \| 2015 \| 2015MNRAS.449.1441K \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.449.1441K Keplers Supernova: An Overluminous Type Ia Event Interacting with a Massive Circumstellar Medium at a Very Late Phase \|Katsuda Satoru Mori Koji et al. \| ApJ \| 808-49 \| 2015 \| 2015ApJ...808...49K \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...808...49K 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 The Interaction of the Fermi Bubbles with the Milky Ways Hot Gas Halo \|Miller Matthew J. Bregman Joel N. \| ApJ \| 829-9 \| 2016 \| 2016ApJ...829....9M \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829....9M 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 Supernova remnants as a probe of dust grains in the interstellar medium \|Williams Brian J. \| PhDT \| 0-132 \| 2010 \| 2010PhDT.......132W \| http://ui.adsabs.harvard.edu/#abs/2010PhDT.......132W 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 Anisotropy of the galaxy cluster X-ray luminosity-temperature relation \|Migkas Konstantinos Reiprich Thomas H. \| A&A \| 611-50 \| 2018 \| 2018A&A...611A..50M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..50M The XMM Cluster Survey: Present status and latest results \|Viana P. T. P. Mehrtens N. et al. \| AN \| 334-462 \| 2013 \| 2013AN....334..462V \| http://ui.adsabs.harvard.edu/#abs/2013AN....334..462V 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 Evolutionary Models for 15 Galactic Supernova Remnants with New Distances \|Leahy D. A. Ranasinghe S. \| ApJ \| 866-9 \| 2018 \| 2018ApJ...866....9L \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...866....9L The Spectrum of the Universe \|Hill Ryley Masui Kiyoshi W. \| ApSpe \| 72-663 \| 2018 \| 2018ApSpe..72..663H \| http://ui.adsabs.harvard.edu/#abs/2018ApSpe..72..663H Supernova remnants in the Magellanic Clouds \|Filipovic M. D. Bozzetto L. M. \| POBeo \| 96-185 \| 2017 \| 2017POBeo..96..185F \| http://ui.adsabs.harvard.edu/#abs/2017POBeo..96..185F Testing emergent gravity on galaxy cluster scales \|Tamosiunas Andrius Bacon David et al. \| JCAP \| 5-53 \| 2019 \| 2019JCAP...05..053T \| http://ui.adsabs.harvard.edu/#abs/2019JCAP...05..053T Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline \|Hollowood Devon L. Jeltema Tesla et al. \| ApJS \| 244-22 \| 2019 \| 2019ApJS..244...22H \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters \|Palmese A. Annis J. et al. \| MNRAS \| 493-4591 \| 2020 \| 2020MNRAS.493.4591P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P 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 An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge \|Qu Zhijie Huang Rui et al. \| ApJ \| 907-14 \| 2021 \| 2021ApJ...907...14Q \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907...14Q 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 Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines \|Qu Zhijie Koutroumpa Dimitra et al. \| ApJ \| 930-21 \| 2022 \| 2022ApJ...930...21Q \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez Antonio C. \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R 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	2000-07-04T05:10:28Z/2002-10-07T17:07:14Z
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	2003-11-14T00:00:00Z
Last Update	2025-01-27
Keywords	"sensitivity spectroscopy", "resolution spectroscopy", "EPIC", "xmm rgs", "thermal spectra", "magellanic clouds ssc_1", "spectral resolution", "thermal supernova remnant", "epic broad band", "xmm epic", "qualify statistical", "spectro imaging", "larger samples", "XMM", "distinguishing lines", "global spectra", "magellanic clouds", "spectral data"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Michael Watson, 2003, 'Spectroscopy of thermal supernova remnants in the Magellanic Clouds SSC_1', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-nmawhut