A dataset provided by the European Space Agency

Name: RXJ1713.7-3946: a unique synchrotron-dominated shell-like SNR
Published: 2009-11-12T00:00:00Z

Proposal ID	055103
Title	RXJ1713.7-3946: a unique synchrotron-dominated shell-like SNR
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0551030101
DOI	https://doi.org/10.5270/esa-kg90pj8
Principal Investigator, PI	Dr Jean Ballet
Abstract	We propose to finish mapping the supernova remnant RX J1713.7-3946 byreobserving one 20 ks pointing which was lost to flaring activity: 1) to obtainthe full and most detailed description of the morphology of the X- raysynchrotron emission to serve as a reference for other wavelengths 2) to comparehow particle acceleration proceeds when the SNR is interacting with molecularclouds or with a tenuous ambient medium 3) to map the material interacting withthe SNR from the variations of the X- ray absorption and compare it to thepotential hadronic gamma-ray emission 4) to map accurately the spectral indexvariations of the X-ray synchrotron emission and look for spatial correlationswith the gamma-ray spectra
Publications	A joint spectro-imaging analysis of the XMM-Newton and HESS observations of the supernova remnant RX J1713.7-3946 \|Acero F. Ballet J. et al. \| A&A \| 505-157 \| 2009 \| 2009A&A...505..157A \| http://ui.adsabs.harvard.edu/#abs/2009A&A...505..157A Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter J. A. Semba S. \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov V. N. \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y Evidence for Thermal X-Ray Line Emission from the Synchrotron-dominated Supernova Remnant RX J1713.7-3946 \|Katsuda Satoru Acero Fabio et al. \| ApJ \| 814-29 \| 2015 \| 2015ApJ...814...29K \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...814...29K 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 H.E.S.S. observations of RX J1713.7-3946 with improved angular and spectral resolution: Evidence for gamma-ray emission extending beyond the X-ray emitting shell \|H. E. S. S. Collaboration Abdalla H. et al. \| A&A \| 612-6 \| 2018 \| 2018A&A...612A...6H \| http://ui.adsabs.harvard.edu/#abs/2018A&A...612A...6H Ground- and Space-Based Gamma-Ray Astronomy \|Funk Stefan \| ARNPS \| 65-245 \| 2015 \| 2015ARNPS..65..245F \| http://ui.adsabs.harvard.edu/#abs/2015ARNPS..65..245F Progressive steepening of the SNR RX J1713.7-3946 X-ray spectrum from XMM-Newton to INTEGRAL \|Kuznetsova Ekaterina Krivonos Roman et al. \| MNRAS \| 489-1828 \| 2019 \| 2019MNRAS.489.1828K \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.489.1828K Evolutionary Models for 43 Galactic Supernova Remnants with Distances and X-Ray Spectra \|Leahy D. A. Ranasinghe S. \| ApJS \| 248-16 \| 2020 \| 2020ApJS..248...16L \| http://ui.adsabs.harvard.edu/#abs/2020ApJS..248...16L A run-wise simulation and analysis framework for Imaging Atmospheric Cherenkov Telescope arrays \|Holler M. Lenain J. -P. et al. \| APh \| 123-102491 \| 2020 \| 2020APh...12302491H \| http://ui.adsabs.harvard.edu/#abs/2020APh...12302491H 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 Pursuing the Origin of the Gamma Rays in RX J1713.7-3946 Quantifying the Hadronic and Leptonic Components \|Fukui Yasuo Sano Hidetoshi et al. \| ApJ \| 915-84 \| 2021 \| 2021ApJ...915...84F \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...915...84F The Gamma-Ray Origin of RX J0852.0-4622 Quantifying the Hadronic and Leptonic Components: Further Evidence for the Cosmic-Ray Acceleration in Young Shell-type SNRs \|Fukui Yasuo Aruga Maki et al. \| ApJ \| 961-162 \| 2024 \| 2024ApJ...961..162F \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...961..162F 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	2008-09-27T16:44:57Z/2008-09-27T23:40:15Z
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	2009-11-12T00:00:00Z
Last Update	2025-01-27
Keywords	"flaring activity", "finish mapping", "particle acceleration proceeds", "synchrotron dominated shell", "xray synchrotron emission", "supernova remnant", "x ray absorption", "spatial correlations", "tenuous ambient medium", "J1713.7", "molecular clouds", "material interacting", "gamma ray spectra", "spectral index variations"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Jean Ballet, 2009, 'RXJ1713.7-3946: a unique synchrotron-dominated shell-like SNR', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-kg90pj8