A dataset provided by the European Space Agency

Name: X-ray identification of the high magnetic field pulsar B1727-47
Published: 2018-04-25T22:00:00Z

Proposal ID	080469
Title	X-ray identification of the high magnetic field pulsar B1727-47
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804690101
DOI	https://doi.org/10.5270/esa-6avuqe0
Principal Investigator, PI	Dr Dima Zyuzin
Abstract	We propose first X-rays observations of the high magnetic field middle-age radiopulsar B1727-47. Models predict that high magnetic field pulsars are hotter thanpulsars with lower magnetic field. However, current X-ray data on highlymagnetized pulsars are scarce to confidently confirm this. Analysis of the radiotiming and interferometry data suggest that B1727-47 has a significant propermotion, which points on the association with the nearby (<1 kpc) evolvedsupernova remnant RCW 114. Potential proximity, high Galactic latitude (b=-7.69deg) and thus low absorption (Nh<2e21 cm-2) make PSR B1727-47 a good X-raytarget to study magnetic field impact on the thermal emission properties ofrotation powered pulsars.
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 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 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	2017-04-05T05:39:44Z/2017-04-05T16:01:24Z
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	2018-04-25T22:00:00Z
Keywords	"thermal emission properties", "lower magnetic field", "xray data", "magnetic field impact", "low absorption nh", "x ray identification", "models predict", "galactic latitude", "psr b1727", "interferometry data", "2e21 cm", "magnetic field pulsars", "potential proximity", "xray target", "magnetized pulsars", "rotation powered pulsars", "proper motion"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Dima Zyuzin, 2018, 'X-ray identification of the high magnetic field pulsar B1727-47', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-6avuqe0