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
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
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
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
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.
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