A dataset provided by the European Space Agency

Name: RX J1713.7-3946: A UNIQUE SYNCHROTRON-DOMINATED SHELL-LIKE SNR
Published: 2005-05-09T00:00:00Z

Proposal ID	020347
Title	RX J1713.7-3946: 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=0203470401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0203470501
DOI	https://doi.org/10.5270/esa-m2k7ok7
Principal Investigator, PI	Mr GAMIL CASSAM-CHENAI
Abstract	We propose to map the supernova remnant (SNR) RX J1713.7-3946 (G347.3-0.5) andits complex environment within 8 pointings of 15 ks to investigate what is themost powerful cosmic-ray accelerator actually known. Our objectives are 1) tomap and diagnostic accurately the spectral variations of the synchrotronemission and to investigate the origin of the TeV emission (in the northwest),2) to determine the morphology and spectral characteristics of the X-ray sourceassociated with the northeast cloud (within the EGRET error box) and itsrelation with the SNR, 3) to compare how particle acceleration proceeds when theSNR is interacting with molecular clouds (in the north) or with tenuous ISM (inthe south), 4) to search for the unrevealed thermal emission over the SNR.
Publications	The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue \|Watson M. G. Schroder A. C. et al. \| A&A \| 493-339 \| 2009 \| 2009A&A...493..339W \| http://ui.adsabs.harvard.edu/#abs/2009A&A...493..339W Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras \|Mateos S. Saxton R. D. et al. \| A&A \| 496-879 \| 2009 \| 2009A&A...496..879M \| http://ui.adsabs.harvard.edu/#abs/2009A&A...496..879M The XMM Cluster Survey: optical analysis methodology and the first data release \|Mehrtens Nicola Romer A. Kathy et al. \| MNRAS \| 423-1024 \| 2012 \| 2012MNRAS.423.1024M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M A Search for New Galactic Magnetars in Archival Chandra and XMM-Newton Observations \|Muno M. P. Gaensler B. M. et al. \| ApJ \| 680-639 \| 2008 \| 2008ApJ...680..639M \| http://ui.adsabs.harvard.edu/#abs/2008ApJ...680..639M An All-Sky Atlas of Radio/X-ray Associations \|Flesch E. \| PASA \| 27-283 \| 2010 \| 2010PASA...27..283F \| http://ui.adsabs.harvard.edu/#abs/2010PASA...27..283F 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 The XMM Cluster Survey: X-ray analysis methodology \|Lloyd-Davies E. J. Romer A. Kathy et al. \| MNRAS \| 418-14 \| 2011 \| 2011MNRAS.418...14L \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.418...14L 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 Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog \|Lin Dacheng Webb Natalie A. \| ApJ \| 756-27 \| 2012 \| 2012ApJ...756...27L \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...27L The XMM-Newton serendipitous ultraviolet source survey catalogue \|Page M. J. Brindle C. et al. \| MNRAS \| 426-903 \| 2012 \| 2012MNRAS.426..903P \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.426..903P Automatic Classification of Time-variable X-Ray Sources \|Lo Kitty K. Farrell Sean et al. \| ApJ \| 786-20 \| 2014 \| 2014ApJ...786...20L \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...786...20L The diversity of quasars unified by accretion and orientation \|Shen Yue Ho Luis C. \| Natur \| 513-210 \| 2014 \| 2014Natur.513..210S \| http://ui.adsabs.harvard.edu/#abs/2014Natur.513..210S 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 Sunyaev-Zeldovich effect or not? Detecting the main foreground effect of most galaxy clusters \|Xiao Weike Chen Chen et al. \| MNRAS \| 432-41 \| 2013 \| 2013MNRAS.432L..41X \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X 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 Anisotropy of the galaxy cluster X-ray luminosity-temperature relation \|Migkas Konstantinos Reiprich Thomas H. \| A&A \| 611-50 \| 2018 \| 2018A&A...611A..50M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..50M 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 The XMM Cluster Survey: Present status and latest results \|Viana P. T. P. Mehrtens N. et al. \| AN \| 334-462 \| 2013 \| 2013AN....334..462V \| http://ui.adsabs.harvard.edu/#abs/2013AN....334..462V X-ray observations of Galactic H.E.S.S. sources: An update \|Puhlhofer G. Eger P. et al. \| AN \| 338-274 \| 2017 \| 2017AN....338..274P \| http://ui.adsabs.harvard.edu/#abs/2017AN....338..274P NuSTAR Observations of the Supernova Remnant RX J1713.7--3946 \|Tsuji Naomi Uchiyama Yasunobu et al. \| ApJ \| 877-96 \| 2019 \| 2019ApJ...877...96T \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...877...96T Testing emergent gravity on galaxy cluster scales \|Tamosiunas Andrius Bacon David et al. \| JCAP \| 5-53 \| 2019 \| 2019JCAP...05..053T \| http://ui.adsabs.harvard.edu/#abs/2019JCAP...05..053T Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline \|Hollowood Devon L. Jeltema Tesla et al. \| ApJS \| 244-22 \| 2019 \| 2019ApJS..244...22H \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H 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 Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters \|Palmese A. Annis J. et al. \| MNRAS \| 493-4591 \| 2020 \| 2020MNRAS.493.4591P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P 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 Radial Profiles of Non-thermal Emission from Supernova Remnant RX J1713.7-3946 \|Tang Yunyong Liu Siming \| ApJ \| 909-46 \| 2021 \| 2021ApJ...909...46T \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...909...46T Systematic Study of Acceleration Efficiency in Young Supernova Remnants with Nonthermal X-Ray Observations \|Tsuji Naomi Uchiyama Yasunobu et al. \| ApJ \| 907-117 \| 2021 \| 2021ApJ...907..117T \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907..117T 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 Multiscale multiwavelength extraction of sources and filaments using separation of the structural components: getsf \|Menshchikov A. \| A&A \| 649-89 \| 2021 \| 2021A&A...649A..89M \| http://ui.adsabs.harvard.edu/#abs/2021A&A...649A..89M 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 Mapping thermal emission in the synchrotron-dominated supernova remnants G330.2+1.0 3C58 and RX J1713.7-3946 \|Picquenot A. Williams B. J. et al. \| A&A \| 683-A197 \| 2024 \| 2024A&A...683A.197P \| http://ui.adsabs.harvard.edu/#abs/2024A&A...683A.197P 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	2004-03-25T08:02:28Z/2004-03-25T18:17:48Z
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	2005-05-09T00:00:00Z
Last Update	2025-01-27
Keywords	"egret error box", "thermal emission", "spectral characteristics", "synchrotron emission", "spectral variations", "3946 g347", "particle acceleration proceeds", "synchrotron dominated shell", "xray source", "northeast cloud", "tev emission", "supernova remnant", "G347.3", "J1713.7", "molecular clouds", "tenuous ism", "rx j1713"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr GAMIL CASSAM-CHENAI, 2005, 'RX J1713.7-3946: A UNIQUE SYNCHROTRON-DOMINATED SHELL-LIKE SNR', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-m2k7ok7