A dataset provided by the European Space Agency

Name: New Candidates for Supernova Remnants in the Large Magellanic Cloud
Published: 2014-05-21T00:00:00Z

Proposal ID	072044
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=0720440101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0720440201
DOI	https://doi.org/10.5270/esa-g8umkd1
Principal Investigator, PI	Dr Manami Sasaki
Abstract	We propose observations of six new candidates for SNRs in the LMC, which weredetected with ROSAT and classified as SNR candidates based on X-ray, radio, andoptical properties. Two sources have already been observed (AO9, Proposal ID65188; AO11, VLP, LMC survey) and confirm the reliability of our selection ofcandidates. The proposed targets are all located outside the LMC VLP survey.Owing to the high sensitivity of XMM-Newton we will be able to detect SNRs thatare X-ray faint either because of their age or the ambient medium and completethe sample of known SNRs to lower flux levels. We will thus be able to performstatistical studies by, e.g., constructing a more complete XLFs of LMC SNRs andwill obtain information about typical abundances, densities, and SN energies.
Publications	XMM-Newton observation of SNR J0533-7202 in the Large Magellanic Cloud \|Kavanagh P. J. Sasaki M. et al. \| A&A \| 579-63 \| 2015 \| 2015A&A...579A..63K \| http://ui.adsabs.harvard.edu/#abs/2015A&A...579A..63K 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 Two evolved supernova remnants with newly identified Fe-rich cores in the Large Magellanic Cloud \|Kavanagh P. J. Sasaki M. et al. \| A&A \| 586-4 \| 2016 \| 2016A&A...586A...4K \| http://ui.adsabs.harvard.edu/#abs/2016A&A...586A...4K 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 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2013-05-03T10:32:42Z/2013-05-09T18:07:53Z
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	2014-05-21T00:00:00Z
Last Update	2025-01-27
Keywords	"lmc survey", "xmm newton", "perform statistical", "supernova remnant", "xray faint", "lmc supernova remnant", "lmc vlp survey", "typical abundance", "magellanic cloud", "id 65188", "lower flux levels", "XMM-Newton", " constructing", "supernova remnant candidates", "ROSAT", "optical properties", "ambient medium", ".", "XMM", "complete xlfs"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Manami Sasaki, 2014, 'New Candidates for Supernova Remnants in the Large Magellanic Cloud', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-g8umkd1