A dataset provided by the European Space Agency

Name: Past history of the S 147 supernova remnant
Published: 2014-04-16T00:00:00Z

Proposal ID	069327
Title	Past history of the S 147 supernova remnant
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693270301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693270401
DOI	https://doi.org/10.5270/esa-gd3weww
Principal Investigator, PI	Dr Jean Ballet
Abstract	S 147 is one of the most spectacular supernova remnants in the optical, and isbelieved to be in the radiative phase. It was recently reported as a relativelybright gamma-ray source by Fermi. In order to interpret the gamma-ray emissioncorrectly, it is important to know whether the accelerated particles are fresh,or the relic from the times when S 147 was younger. The amount and spectrum ofthe relic particles depend on the past history of the density and shockvelocity. The hot gas still trapped inside the remnant stands witness to that.Building on a marginal detection in the ROSAT survey, we propose an XMM-Newtonobservation to determine the temperature and density inside S 147.
Publications	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 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 The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII O VIII and Fe L-shell Transitions \|Pan Zeyang Qu Zhijie et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P 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	2013-02-27T04:44:41Z/2013-04-04T21:02:37Z
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	2014-04-16T00:00:00Z
Last Update	2025-01-27
Keywords	"density inside", "relic particles depend", "trapped inside", "radiative phase", "marginal detection", "xmm newton", "147 supernova remnant", "spectacular supernova remnant", "remnant stands", "XMM-Newton", "shock velocity", "ROSAT", "past history", "XMM", "rosat survey", "hot gas", "accelerated particles"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Jean Ballet, 2014, 'Past history of the S 147 supernova remnant', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-gd3weww