A dataset provided by the European Space Agency

Name: Completing the X-ray view of the Supernova Remnant Puppis A
Published: 2013-06-16T00:00:00Z

Proposal ID	069097
Title	Completing the X-ray view of the Supernova Remnant Puppis A
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690970101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0690970201
DOI	https://doi.org/10.5270/esa-3b55i3t
Principal Investigator, PI	Dr Gloria Dubner
Abstract	Despite a large fraction of the SNR Puppis A having been observed in X-rays,there is a distinct scarcity of data in the southern extent of the remnant. Todate, the highest quality X-ray exposures of the South are those of theXMM-Newton Slew Survey, which confirm the existence of X-ray emission associatedwith the SNR. Moreover, high sensitivity radio data show that the South is aregion of high interest due to its likely interaction with neighbouring clouds.This proposal aims towards a completion of our view of Puppis A through thefirst deep X-ray observation of the S and SW extent of the remnant.
Publications	The most complete and detailed X-ray view of the SNR Puppis A \|Dubner G. Loiseau N. et al. \| A&A \| 555-9 \| 2013 \| 2013A&A...555A...9D \| http://ui.adsabs.harvard.edu/#abs/2013A&A...555A...9D 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 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 Rectangular core-collapse supernova remnants: application to Puppis A \|Meyer D. M. -A. Velu00e1zquez P. F. et al. \| MNRAS \| 515-594 \| 2022 \| 2022MNRAS.515..594M \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.515..594M Progenitors and explosion properties of supernova remnants hosting central compact objects: II. A global systematic study with a comparison to nucleosynthesis models \|Braun C. Safi-Harb S. et al. \| MNRAS \| 525-6257 \| 2023 \| 2023MNRAS.525.6257B \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.525.6257B 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 Progenitors and Explosion Properties of Supernova Remnants Hosting Central Compact Objects \|Braun Chelsea \| PhDT \| 0-5 \| 2023 \| 2023PhDT.........5B \| http://ui.adsabs.harvard.edu/#abs/2023PhDT.........5B New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2012-05-05T05:18:05Z/2012-06-03T16:31:27Z
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	2013-06-16T00:00:00Z
Last Update	2025-08-04
Keywords	"XMM", "aims towards", "XMM-Newton", "quality xray", "southern extent", "supernova remnant puppis", "sensitivity radio data", "distinct scarcity", "sw extent", "xray emission", "deep xray", "neighbouring clouds", "supernova remnant"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Gloria Dubner, 2013, 'Completing the X-ray view of the Supernova Remnant Puppis A', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-3b55i3t