A dataset provided by the European Space Agency

Name: New Candidates for Supernova Remnants in the Large Magellanic Cloud
Published: 2015-06-30T22:00:00Z

Proposal ID	074180
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=0741800101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0741800201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0741800301
DOI	https://doi.org/10.5270/esa-u2s04kc
Principal Investigator, PI	Dr Patrick Kavanagh
Abstract	We propose observations of five new candidates for X-ray supernova remnants(SNRs) in the Large Magellanic Cloud (LMC), which were detected in ROSAT dataand classified as SNR candidates based on their X-ray, radio, and opticalproperties. Five sources have already been observed (AO9 and AO12, Prop. IDs65188 and 72044; AO11, VLP-LMC survey) and confirm the reliability of ourcandidate selection. The high sensitivity of XMM-Newton will allow us to detectSNRs that are X-ray faint due to their age or ambient medium, and complete thesample of known SNRs to lower fluxes. We will thus be able to performstatistical studies by, e.g., constructing a more complete X-ray luminosityfunction of SNRs in the LMC and will obtain information about typical abundances, densities, and initial supernova energies.
Publications	Multi-frequency study of the newly confirmed supernova remnant MCSNR J0512-6707 in the Large Magellanic Cloud \|Kavanagh P. J. Sasaki M. et al. \| A&A \| 583-121 \| 2015 \| 2015A&A...583A.121K \| http://ui.adsabs.harvard.edu/#abs/2015A&A...583A.121K 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 EXTraS discovery of two pulsators in the direction of the LMC: a Be/X-ray binary pulsar in the LMC and a candidate double-degenerate polar in the foreground \|Haberl F. Israel G. L. et al. \| A&A \| 598-69 \| 2017 \| 2017A&A...598A..69H \| http://ui.adsabs.harvard.edu/#abs/2017A&A...598A..69H Statistical Analysis of Supernova Remnants in the Large Magellanic Cloud \|Bozzetto Luke M. Filipovic Miroslav D. et al. \| ApJS \| 230-2 \| 2017 \| 2017ApJS..230....2B \| http://ui.adsabs.harvard.edu/#abs/2017ApJS..230....2B 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 Detection of a 23.6 min periodic modulation in the optical counterpart of 3XMMJ051034.6-670353 \|Ramsay G. Marsh T. R. et al. \| A&A \| 617-88 \| 2018 \| 2018A&A...617A..88R \| http://ui.adsabs.harvard.edu/#abs/2018A&A...617A..88R The supernova remnant population of the Small Magellanic Cloud \|Maggi Pierre Filipoviu0107 Miroslav D. et al. \| A&A \| 631-127 \| 2019 \| 2019A&A...631A.127M \| http://ui.adsabs.harvard.edu/#abs/2019A&A...631A.127M 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 Spitzer and Herschel studies of dust in supernova remnants in the Small Magellanic Cloud \|Matsuura Mikako Ayley Victoria et al. \| MNRAS \| 513-1154 \| 2022 \| 2022MNRAS.513.1154M \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.513.1154M New XMM-Newton observations of faint evolved supernova remnants in the Large Magellanic Cloud \|Kavanagh P. J. Sasaki M. et al. \| MNRAS \| 515-4099 \| 2022 \| 2022MNRAS.515.4099K \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.515.4099K 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	2014-05-17T01:56:25Z/2014-06-08T14:16:33Z
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	2015-06-30T22:00:00Z
Last Update	2025-01-27
Keywords	"perform statistical", "xmm newton", "supernova remnant", "xray faint", "typical abundance", "magellanic cloud", "initial supernova energies", "lower fluxes", "rosat data", "XMM-Newton", " constructing", "magellanic cloud lmc", "vlp lmc survey", "supernova remnant candidates", "ROSAT", "candidate selection", "optical properties", "ambient medium", ".", "XMM", "ids 65188"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Patrick Kavanagh, 2015, 'New Candidates for Supernova Remnants in the Large Magellanic Cloud', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-u2s04kc