A dataset provided by the European Space Agency

Name: New Candidates for Supernova Remnants in the Large Magellanic Cloud
Published: 2016-09-14T22:00:00Z

Proposal ID	076406
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=0764060101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0764060201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0764060301
DOI	https://doi.org/10.5270/esa-1eq40pn
Principal Investigator, PI	Dr Patrick Kavanagh
Abstract	We propose observations of four candidates for X-ray supernova remnants (SNRs)in the Large Magellanic Cloud (LMC), which were detected by ROSAT and classifiedas SNR candidates based on their X-ray, radio and optical properties. Sevensources have already been observed (AO9, AO12, and AO13, Prop. IDs 65188, 72044,74180; AO11, VLP-LMC survey) and confirm the reliability of our candidateselection. The high sensitivity of XMM-Newton will allow us to detect SNRs thatare X-ray faint due to their age or ambient medium, and complete the sample ofknown SNRs to lower fluxes. We will be able to perform statistical studies by,e.g., constructing a more complete X-ray luminosity function of SNRs in the LMCand will obtain information about typical abundances, densities, and supernova energies.
Publications	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 nature of 50 Palermo Swift-BAT hard X-ray objects through optical spectroscopy \|Rojas A. F. Masetti N. et al. \| A&A \| 602-124 \| 2017 \| 2017A&A...602A.124R \| http://ui.adsabs.harvard.edu/#abs/2017A&A...602A.124R 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 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 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	2015-06-20T11:52:27Z/2015-08-19T14:53:22Z
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	2016-09-14T22:00:00Z
Last Update	2025-01-27
Keywords	"perform statistical", "xmm newton", "supernova remnant", "xray faint", "typical abundance", "magellanic cloud", "lower fluxes", "XMM-Newton", " constructing", "magellanic cloud lmc", "vlp lmc survey", "supernova remnant candidates", "ROSAT", "candidate selection", "supernova energies", "optical properties", "ambient medium", "XMM", ".", "ids 65188"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Patrick Kavanagh, 2016, 'New Candidates for Supernova Remnants in the Large Magellanic Cloud', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-1eq40pn