A dataset provided by the European Space Agency

Name: In-depth investigation of the two oldest type Ia supernova remnants in the LMC
Published: 2015-05-29T22:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	074430
Title	In-depth investigation of the two oldest type Ia supernova remnants in the LMC
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744300101
DOI	https://doi.org/10.5270/esa-543x2du
Principal Investigator, PI	Mr Pierre Maggi
Abstract	We propose observations of 2 type Ia SNRs in the LMC. The targets have beenserendipitously discovered at high off-axis angles in the XMM survey of the LMC,and appear to be the most evolved type Ia SNRs. Deep on-axis observations willprovide key information in the study of type Ia SNe and their progenitors, andhelp us to understand the latest stage of a remnant. We will refine themeasurement of the mass of Fe present in the remnants, and probe the centralenvironment of type Ia SNRs. Improved X-ray images will enable the search for asurviving companion, and the study of spatio-spectral variations, revealingpossible asymmetry of the SN explosion or ejecta stratification. Finally, faintX-ray shells can be detected, providing measurements of, or limits on, the age of the remnants.
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 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 A new multiwavelength census of blazars \|Paggi A. Bonato M. et al. \| A&A \| 641-62 \| 2020 \| 2020A&A...641A..62P \| http://ui.adsabs.harvard.edu/#abs/2020A&A...641A..62P 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 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	2014-05-03T09:32:44Z/2014-05-04T10:30:34Z
Version	21.51_20241115_1113
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	2015-05-29T22:00:00Z
Last Update	2026-07-09
Keywords	"improved xray images", "type ia sne", "depth investigation", "faint xray shells", "ejecta stratification", "spatio spectral variations", "XMM", "xmm survey", "axis angles", "surviving companion", "key information"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr Pierre Maggi, 2015, 'In-depth investigation of the two oldest type Ia supernova remnants in the LMC', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-543x2du
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.