A dataset provided by the European Space Agency

Name: XMM-RGS Spectroscopy of the Magellanic Cloud Supernova Remnant Sample.
Published: 2003-01-04T00:00:00Z

Proposal ID	011300
Title	XMM-RGS Spectroscopy of the Magellanic Cloud Supernova Remnant Sample.
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0113000201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0113000301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0113000401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0113000501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0113000601
DOI	https://doi.org/10.5270/esa-7to9arn
Principal Investigator, PI	Dr Albert Brinkman
Abstract	GT- We propose to observe a sample of the supernova remnants in the MagellanicClouds. The sample is comprised of E0102-72.3, N49, N103B, PSR0540-69.3 and 0519-69.0. These SNRs form a biased sample of the SNR population (they are drawn from the brighter and smaller ends of the distribution), but the sample spans the spectrum of origin, age and dynamical conditions: Two are type Ia, two are type II (one with a pulsar) and the other is evolved and containing a known soft gamma repeater. This set, studied using the RGS, promises unambiguous spectra and line diagnostics that provide strong clues that address the composition and physical state of the interstellar medium withinthe MCs, as well as that of the ejected stellar material.
Publications	High-Resolution X-ray imaging and spectroscopy of N 103B \|van der Heyden, K. J., Behar, E., et al. \| A&A \| 392-955 \| 2002 \| 2002A&A...392..955V \| http://ui.adsabs.harvard.edu/#abs/2002A&A...392..955V 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 Supernova Remnants in the Magellanic Clouds. IX. Multiwavelength Analysis of the Physical Structure of N49 \|Bilikova, J., Williams, R. N. M., et al. \| AJ \| 134-2308 \| 2007 \| 2007AJ....134.2308B \| http://ui.adsabs.harvard.edu/#abs/2007AJ....134.2308B 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 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 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 The kinematics and chemical stratification of the type Ia supernova remnant 0519-69.0. An XMM-Newton and Chandra study \|Kosenko, D., Helder, E. A., \| A&A \| 519-11 \| 2010 \| 2010A&A...519A..11K \| http://ui.adsabs.harvard.edu/#abs/2010A&A...519A..11K Evolution of X-ray emission from young massive star clusters \|Oskinova, L. M., \| MNRAS \| 361-679 \| 2005 \| 2005MNRAS.361..679O \| http://ui.adsabs.harvard.edu/#abs/2005MNRAS.361..679O 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 Mining for normal galaxies in the first XMM-Newton Serendipitous Source Catalog \|Georgakakis, A. E., Chavushyan, V., et al. \| MNRAS \| 367-1017 \| 2006 \| 2006MNRAS.367.1017G \| http://ui.adsabs.harvard.edu/#abs/2006MNRAS.367.1017G 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 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 The Discovery of an X-Ray/UV Stellar Flare from the Late-K/Early-M Dwarf LMC 335 \|Tsang, B. T. H., Pun, C. S. J., et al. \| ApJ \| 754-107 \| 2012 \| 2012ApJ...754..107T \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...754..107T 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 Supernova remnants: the X-ray perspective \|Vink, Jacco, \| A&ARv \| 20-49 \| 2012 \| 2012A&ARv..20...49V \| http://ui.adsabs.harvard.edu/#abs/2012A&ARv..20...49V 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 XMM-Newton serendipitous source catalogue \|Watson, M. G., Pye, J. P., et al. \| AN \| 324-89 \| 2003 \| 2003AN....324...89W \| http://ui.adsabs.harvard.edu/#abs/2003AN....324...89W 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 Automatic Classification of Time-variable X-Ray Sources \|Lo, Kitty K., Farrell, Sean, et al. \| ApJ \| 786-20 \| 2014 \| 2014ApJ...786...20L \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...786...20L 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-Zel.dovich 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 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 A Modern Search for Wolf-Rayet Stars in the Magellanic Clouds: First Results \|Massey, Philip, Neugent, Kathryn F., et al. \| ApJ \| 788-83 \| 2014 \| 2014ApJ...788...83M \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...788...83M The Interaction of the Fermi Bubbles with the Milky Way.s 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 Chandra and XMM-Newton: Synergies now and in the future \|Wilkes, B. J., \| AN \| 338-140 \| 2017 \| 2017AN....338..140W \| http://ui.adsabs.harvard.edu/#abs/2017AN....338..140W 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 Evidence for Resonance Scattering in the X-Ray Grating Spectrum of the Supernova Remnant N49 \|Amano, Yuki, Uchida, Hiroyuki, et al. \| ApJ \| 897-12 \| 2020 \| 2020ApJ...897...12A \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...897...12A 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 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 Discovery of Double-ring Structure in the Supernova Remnant N103B: Evidence for Bipolar Winds from a Type Ia Supernova Progenitor \|Yamaguchi, Hiroya, Acero, Fabio, et al. \| ApJ \| 910-24 \| 2021 \| 2021ApJ...910L..24Y \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...910L..24Y 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 XMMU J050722.1-684758: discovery of a new Be X-ray binary pulsar likely associated with the supernova remnant MCSNR J0507-6847 \|Maitra, C., Haberl, F., et al. \| MNRAS \| 504-326 \| 2021 \| 2021MNRAS.504..326M \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.504..326M The EXTraS project: Exploring the X-ray transient and variable sky \|De Luca, A., Salvaterra, R., et al. \| A&A \| 650-167 \| 2021 \| 2021A&A...650A.167D \| http://ui.adsabs.harvard.edu/#abs/2021A&A...650A.167D 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	2000-07-07T03:09:54Z/2001-09-18T01:26:07Z
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	2003-01-04T00:00:00Z
Keywords	"xmm rgs spectroscopy", "e0102 72", "supernova remnant", "XMM", "biased sample", "supernova remnant form", "dynamical conditions", "promises unambiguous spectra", "supernova remnant population", "type ii", "soft gamma repeater", "line diagnostics", "type ia", "sample spans", "interstellar medium", "magellanic clouds", "stellar material"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Albert Brinkman, 2003, 'XMM-RGS Spectroscopy of the Magellanic Cloud Supernova Remnant Sample.', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-7to9arn