A dataset provided by the European Space Agency

Name: The Origin of a Possible Pulsar Wind Nebula in the Cygnus Loop
Published: 2014-06-18T00:00:00Z

Proposal ID	072213
Title	The Origin of a Possible Pulsar Wind Nebula in the Cygnus Loop
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0722130101
DOI	https://doi.org/10.5270/esa-5hlvkv4
Principal Investigator, PI	Dr Robert Petre
Abstract	The Cygnus Loop is one of the brightest, nearest (d sim 540pc), and mostextensively studied supernova remnants. There are numerous observationalindications that it originated from a core-collapse supernova whose progenitormass is sim 15,M _odot . Nevertheless, no neutron star related to the remnanthas yet been identified. A thorough {it Suzaku} XIS mapping of the Cygnus Loophas revealed a possible pulsar wind nebula (PWN) in the Loop. We propose a100,ks EPIC observation of the candidate PWN in order to determine whether ornot it is associated with the Cygnus Loop by measuring the neutron star propermotion and the column density to the nebula. This observation also will allow usto perform spectral mapping to characterize the PWN and constrain the neutron star pulse period.
Publications	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 No Pulsar Wind Nebula in the Southern Blowout Region of the Cygnus Loop \|Halpern, J. P., Gotthelf, E. V., \| ApJ \| 882-155 \| 2019 \| 2019ApJ...882..155H \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...882..155H 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	2013-05-31T10:12:05Z/2013-06-01T17:02:44Z
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	2014-06-18T00:00:00Z
Keywords	"progenitor mass", "neutron star related", "supernova remnant", "core collapse supernova", "_odot $.", "candidate pwn", "perform spectral mapping", "cygnus loop", "xis mapping", "EPIC", "pulsar wind nebula", "column density"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Robert Petre, 2014, 'The Origin of a Possible Pulsar Wind Nebula in the Cygnus Loop', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-5hlvkv4