A dataset provided by the European Space Agency

Name: New Candidates for Supernova Remnants in the Large Magellanic Cloud
Published: 2011-06-25T00:00:00Z

Proposal ID	065188
Title	New Candidates for Supernova Remnants in the Large Magellanic Cloud
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0651880101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0651880201
DOI	https://doi.org/10.5270/esa-bif5thv
Principal Investigator, PI	Dr Manami Sasaki
Abstract	We propose observations of nine NEW candidates for SNRs in the LMC. Thesesources were detected in ROSAT data and classified as candidates for thermalSNRs based on their X-ray properties and radio counterparts. Using EPICs as theprimary instruments we will detect emission lines of ionized atomscharacteristic of thermal SNRs and determine the spatial extent. The highsensitivity of XMM-Newton will allow to detect SNRs that are X-ray faint eitherbecause of their age or the ambient medium and enlarge the sample of known SNRsto lower brightness levels. We will thus be able to construct a more completeX-ray luminosity function of SNRs in the LMC and will obtain information abouttypical abundances, densities, and initial supernova energies in the LMC.
Publications	XMMU J0541.8-6659 a new supernova remnant in the Large Magellanic Cloud \|Grondin M.-H. Sasaki M. et al. \| A&A \| 539-15 \| 2012 \| 2012A&A...539A..15G \| http://ui.adsabs.harvard.edu/#abs/2012A&A...539A..15G Multifrequency study of a new Fe-rich supernova remnant in the Large Magellanic Cloud MCSNR J0508-6902 \|Bozzetto L. M. Kavanagh P. J. et al. \| MNRAS \| 439-1110 \| 2014 \| 2014MNRAS.439.1110B \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.439.1110B 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 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 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 AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton \|Svoboda J. Guainazzi M. \| A&A \| 603-127 \| 2017 \| 2017A&A...603A.127S \| http://ui.adsabs.harvard.edu/#abs/2017A&A...603A.127S 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 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 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 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 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 New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2010-05-02T08:38:20Z/2010-06-06T10:01:03Z
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	2011-06-25T00:00:00Z
Last Update	2025-08-04
Keywords	"radio counterparts", "rosat data", "emission lines", "initial supernova energies", "supernova remnant", "XMM", "lower brightness levels", "xray properties", "spatial extent", "xmm newton", "ambient medium", "ionized atoms characteristic", "xray faint", "XMM-Newton", "magellanic cloud", "ROSAT", "EPIC", "typical abundance", "thermal supernova remnant", "primary instruments"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Manami Sasaki, 2011, 'New Candidates for Supernova Remnants in the Large Magellanic Cloud', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-bif5thv