A dataset provided by the European Space Agency

Name: Establishing the conditions for high-energy emission around supernova G22.7-0.2
Published: 2012-04-01T00:00:00Z

Proposal ID	065448
Title	Establishing the conditions for high-energy emission around supernova G22.7-0.2
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0654480101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0654480201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0654480301
DOI	https://doi.org/10.5270/esa-ayqxjoi
Principal Investigator, PI	Dr Andre-Claude Clapson
Abstract	SNR G22.7-0.2 is a well-resolved shell (26 in diameter), observed in a largemulti-wavelength dataset. It is possibly in interaction with the adjacent SNRG23.3-0.3, with likely consequences for high-energy particle production. Thesecircumstances make this SNR a good candidate for a detailed study in the keVband, which is still missing. We propose a full coverage of the SNR shell withemph{XMM-Newton}, to complete the characterization of its parameters, startingwith its age and distance, as well as to map the properties of non-thermalparticles around its shell and study the proposed SNR-SNR interaction region.
Publications	Discovery of the VHE gamma-ray source HESS J1832-093 in the vicinity of SNR G22.7-0.2 \|HESS Collaboration Abramowski A. et al. \| MNRAS \| 446-1163 \| 2015 \| 2015MNRAS.446.1163H \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.446.1163H 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 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 NuSTAR Hard X-Ray Observation of the Gamma-Ray Binary Candidate HESS J1832-093 \|Mori Kaya Gotthelf E. V. et al. \| ApJ \| 848-80 \| 2017 \| 2017ApJ...848...80M \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...848...80M 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 X-ray and u03b3-ray orbital variability from the u03b3-ray binary HESS J1832-093 \|Martu00ed-Devesa G. Reimer O. \| A&A \| 637-23 \| 2020 \| 2020A&A...637A..23M \| http://ui.adsabs.harvard.edu/#abs/2020A&A...637A..23M 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 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	2010-09-26T23:02:19Z/2011-03-13T16:41:25Z
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	2012-04-01T00:00:00Z
Keywords	"", "xmm newton }", "supernova remnant shell", "G22.7", "supernova remnant", "energy particle production", "XMM", "nonthermal particles", "energy emission", "multi wavelength dataset", "supernova g22", "supernova remnant g22", "XMM-Newton", "resolved shell", "kev band"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Andre-Claude Clapson, 2012, 'Establishing the conditions for high-energy emission around supernova G22.7-0.2', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ayqxjoi