A dataset provided by the European Space Agency

Name: Exploring cosmic-ray acceleration environment in the SNR CTB37B
Published: 2011-04-24T00:00:00Z

Proposal ID	060602
Title	Exploring cosmic-ray acceleration environment in the SNR CTB37B
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0606020101
DOI	https://doi.org/10.5270/esa-9k5dyp9
Principal Investigator, PI	Ms Ryoko Nakamura
Abstract	Although cosmic rays are accelerated at the shock front of supernova remnants(SNRs), condition for the particle accelation to occur is poorly understood. Oneof the ways to resolve this problem is to investigate thermal X-ray emissionassociated with the acceleration site, because the thermal emission provides usthe information of the condistions. We propose XMM-Newton of the SNR CTB37Bwhich has thermal, non-thermal X-ray and TeV I?-ray emission. Suzaku and Chandraobservations could not determine the parameters of the thermal plasma because ofthe contamination of a point source and of statistical limitation. Only goodspatial resolution and large effective area of XMM-Newton enable us toinvestigate the thermal X-ray emission.
Publications	Identification of CXOU J171405.7-381031 as a New Magnetar with XMM-Newton \|Sato Takuro Bamba Aya et al. \| PASJ \| 62-33 \| 2010 \| 2010PASJ...62L..33S \| http://ui.adsabs.harvard.edu/#abs/2010PASJ...62L..33S Unifying the observational diversity of isolated neutron stars via magneto-thermal evolution models \|Vigano D. Rea N. et al. \| MNRAS \| 434-123 \| 2013 \| 2013MNRAS.434..123V \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.434..123V 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 X-Ray Perspective of the Twisted Magnetospheres of Magnetars \|Weng Shan-Shan Gogus Ersin et al. \| ApJ \| 805-81 \| 2015 \| 2015ApJ...805...81W \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...805...81W 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 Magnetic fields in neutron stars \|Vigano Daniele \| PhDT \| 0-7 \| 2013 \| 2013PhDT.........7V \| http://ui.adsabs.harvard.edu/#abs/2013PhDT.........7V An Energetic Magnetar in HESS J1713-381/CTB 37B \|Halpern J. P. Gotthelf E. V. \| ApJ \| 725-1384 \| 2010 \| 2010ApJ...725.1384H \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...725.1384H XMM-Newton spectrum of the magnetar CXOU J171405.7-381031 \|Watanabe Haruka Bamba Aya et al. \| PASJ \| 71-84 \| 2019 \| 2019PASJ...71...84W \| http://ui.adsabs.harvard.edu/#abs/2019PASJ...71...84W X-ray and radio studies of SNR CTB 37B hosting the magnetar CXOU J171405.7-381031 \|Blumer Harsha Safi-Harb Samar et al. \| MNRAS \| 487-5019 \| 2019 \| 2019MNRAS.487.5019B \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.487.5019B X-Ray Monitoring of the Magnetar CXOU J171405.7-381031 in Supernova Remnant CTB 37B \|Gotthelf E. V. Halpern J. P. et al. \| ApJ \| 882-173 \| 2019 \| 2019ApJ...882..173G \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...882..173G 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	2010-03-17T13:16:16Z/2010-03-18T23:06:33Z
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	2011-04-24T00:00:00Z
Last Update	2025-01-27
Keywords	"thermal emission", "shock front", "cosmic rays", "acceleration site", "ray emission", "supernova remnant ctb37b", "nonthermal xray", "xmm newton", "thermal plasma", "XMM-Newton", "thermal xray emission", "XMM", "particle accelation", "statistical limitation", "spatial resolution"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Ms Ryoko Nakamura, 2011, 'Exploring cosmic-ray acceleration environment in the SNR CTB37B', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-9k5dyp9