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
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	2025-01-27
Keywords	"quality xray", "sensitivity radio data", "neighbouring clouds", "distinct scarcity", "supernova remnant", "XMM-Newton", "sw extent", "aims towards", "xray emission", "XMM", "deep xray", "supernova remnant puppis", "southern extent"
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