A dataset provided by the European Space Agency

Name: Search for CCOs in two Galactic SNRs and their first X-ray characterization
Published: 2018-05-25T22:00:00Z

Proposal ID	080345
Title	Search for CCOs in two Galactic SNRs and their first X-ray characterization
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0803450201
DOI	https://doi.org/10.5270/esa-q0rbfwj
Principal Investigator, PI	Dr Dmitry Klochkov
Abstract	We propose to observe two Galactic supernova remnants (SNRs) G 94.0+1.0(3C434.1) and G,96.0+2.0 which have so far not been characterized in X-rays butare well suited for an XMM-Newton study. We plan to search for possible centralneutron stars (NS) associated with the remnants, i.e. to increase the small butdiverse class of isolated NSs associated with SNRs (which is believed to includemagnetars, anti-magnetars, young energetic pulsars with rich phenomena), andto perform the first morphological and spectral study of the remnants in X-rays.The target SNRs are located relatively far from the Galactic center
Publications	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	2017-05-05T04:25:46Z/2017-05-05T14:57:26Z
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	2018-05-25T22:00:00Z
Keywords	"", "target supernova remnant", "supernova remnant", "XMM", "diverse class", "xray characterization", "magnetar "", "galactic supernova remnant", "located relatively", "galactic center", "rich phenomena", "energetic pulsars", "XMM-Newton", "isolated nss", "anti magnetar "", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Dmitry Klochkov, 2018, 'Search for CCOs in two Galactic SNRs and their first X-ray characterization', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-q0rbfwj