A dataset provided by the European Space Agency

Name: IGR J17448-3232: a young, non-thermal supernova remnant?
Published: 2013-03-24T00:00:00Z

Proposal ID	067226
Title	IGR J17448-3232: a young, non-thermal supernova remnant?
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0672260101
DOI	https://doi.org/10.5270/esa-gbua8e7
Principal Investigator, PI	Dr John Tomsick
Abstract	The study of young supernova remnants (SNRs) is important for understanding theparticle acceleration that leads to cosmic ray production, for learning aboutsupernova explosions, and for using energetic pulsars to constrain high energyemission mechanisms. IGR J17448-3232 is a SNR candidate that would be one ofonly three SNRs that have been discovered by the INTEGRAL satellite in the hardX-ray band. The evidence that the source is a SNR comes from short Chandra andSwift exposures that show a source that is several arcminutes in size. Theevidence that it is young comes from its very hard X-ray spectrum. We proposefor an XMM-Newton observation to determine the morphology and spectralproperties of the extended emission.
Publications	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 Source Identification in the IGR J17448-3232 Field: Discovery of the Scorpius Galaxy Cluster \|Barriere Nicolas M. Tomsick John A. et al. \| ApJ \| 799-24 \| 2015 \| 2015ApJ...799...24B \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...799...24B 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 Characterization of diffuse X-ray emission from IGR J17448-3232: an implication of a line-of-sight merging activity \|Watanabe Shoko Yamauchi Shigeo et al. \| PASJ \| 71-116 \| 2019 \| 2019PASJ...71..116W \| http://ui.adsabs.harvard.edu/#abs/2019PASJ...71..116W 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	2012-02-26T04:16:42Z/2012-02-26T16:28:41Z
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	2013-03-24T00:00:00Z
Last Update	2025-01-27
Keywords	"igr j17448 3232", "xmm newton", "hard xray band", "supernova remnant", "XMM-Newton", "supernova remnant candidate", "particle acceleration", "spectral properties", "integral satellite", "hard xray spectrum", "energy emission mechanisms", "XMM", "energetic pulsars", "supernova remnant comes", "cosmic ray production", "short chandra", "supernova explosions"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr John Tomsick, 2013, 'IGR J17448-3232: a young, non-thermal supernova remnant?', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-gbua8e7