A dataset provided by the European Space Agency

Name: In-depth investigation of one of the most evolved type Ia SNR in the LMC
Published: 2016-06-26T22:00:00Z

Proposal ID	076382
Title	In-depth investigation of one of the most evolved type Ia SNR in the LMC
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763820101
DOI	https://doi.org/10.5270/esa-ax1cg20
Principal Investigator, PI	Mr Pierre Maggi
Abstract	We propose a deep observation of a type Ia SNR in the LMC, serendipitouslydiscovered at high off-axis angles in the XMM-Newton survey of the LMC. Itappears to be one of the most evolved type Ia SNR. A deep on-axis observationwill provide key information in the study of type Ia SNe and their progenitors,and help us to understand the latest stage of a remnant. We will be able torefine the measurement of the mass of Fe present in the remnant, and probe theprogenitors circumstellar medium. Improved X-ray images will enable the searchfor a surviving companion, and the study of the distribution of ejecta,revealing possible asymmetries of the SN explosion. Finally, a faint X-ray shellcan be detected, providing measurement of, or limits on, the age of the remnant or ambient density.
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 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 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	2015-06-08T10:07:30Z/2015-06-09T09:59:09Z
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	2016-06-26T22:00:00Z
Last Update	2025-01-27
Keywords	"surviving companion", "axis angles", "circumstellar medium", "key information", "depth investigation", "XMM-Newton", "faint xray shell", "ambient density", "improved xray images", "XMM", "type ia sne", "xmm newton survey"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr Pierre Maggi, 2016, 'In-depth investigation of one of the most evolved type Ia SNR in the LMC', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ax1cg20