A dataset provided by the European Space Agency

Name: Observations of PKS 1209-5152: A Cygnus Loop SiblingquestionMark
Published: 2017-07-15T22:00:00Z

Proposal ID	078172
Title	Observations of PKS 1209-5152: A Cygnus Loop Sibling?
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0781720101
DOI	https://doi.org/10.5270/esa-yxj2z7l
Principal Investigator, PI	Dr Brian Williams
Abstract	The number of SNRs older than 10,000 yr well-studied in X-rays is small, due tothe observational difficulties of mapping low surface brightness thermal plasmaswith temperatures of a few tenths of a keV with interstellar absorption. Wepropose to observe the bright limb of G296.5+10.0, also known as PKS 1209-51/52,with the EPIC instruments. We will produce a map of the bright, soft, thermalemission along the southeastern shell, to be compared with optical, radio, andCO continuum maps. We will characterize the temperature and density variationsin the shell, which result from interactions between the forward shock andstructures in the ISM. A more complete understanding of the old, very large SNRswill help us understand the feedback role that SNe play in the evolution of the Galactic ISM.
Publications	TeV Cosmic-Ray Nucleus Acceleration in Shell-type Supernova Remnants with Hard \\u03b3-Ray Spectra \|Zeng, Houdun, Xin, Yuliang, et al. \| ApJ \| 910-78 \| 2021 \| 2021ApJ...910...78Z \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...910...78Z 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 Observaciones del remanente de supernova G296.5+10.0 con el sat\\u00e9lite XMM-Newton \|Eppens, L. K., Combi, J. A., \| BAAA \| 63-152 \| 2022 \| 2022BAAA...63..152E \| http://ui.adsabs.harvard.edu/#abs/2022BAAA...63..152E The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions \|Pan, Zeyang, Qu, Zhijie, et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P A high-energy study of the supernova remnant G296.5+10.0 \|Eppens, L. K., Combi, J. A., et al. \| MNRAS \| 528-2095 \| 2024 \| 2024MNRAS.528.2095E \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.528.2095E 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	2016-06-27T16:03:47Z/2016-06-27T23:50:27Z
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	2017-07-15T22:00:00Z
Keywords	"southeastern shell", "sne play", "epic instruments", "supernova remnant", "G296.5", "000 yr", "galactic ism", "forward shock", "co continuum maps", "1209 5152", "bright limb", "EPIC", "interstellar absorption", "thermal emission", "feedback role", "density variations"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Brian Williams, 2017, 'Observations of PKS 1209-5152: A Cygnus Loop SiblingquestionMark', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-yxj2z7l