A dataset provided by the European Space Agency

Name: Mapping the Emission Structure of the Brightest Magnetar, 1E 1841-045
Published: 2018-04-20T22:00:00Z

Proposal ID	078308
Title	Mapping the Emission Structure of the Brightest Magnetar, 1E 1841-045
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783080101
DOI	https://doi.org/10.5270/esa-caov8zy
Principal Investigator, PI	Prof Ersin Gogus
Abstract	We propose a deep 80 ks observations of the magnetar, 1E 1841-045 in order toperform phase resolved spectral analysis using physical magnetar emissionmodels. With this observation we will be able to construct the surfacetemperature and magnetic field topology, as well as the magnetospheric structureof this unique magnetar. Given that the persistent X-ray emission properties of1E 1841-045 do not vary significantly, we will employ recent NuSTARobservations, and perform broadband (0.5-79 keV) X-ray spectroscopy of thesource. We will also be able to search for phase dependent spectral features andlow level magnetar bursts from 1E 1841-045 with this data set.
Publications	Supernova remnants with magnetars: Clues to magnetar formation \|Vink Jacco \| AdSpR \| 41-503 \| 2008 \| 2008AdSpR..41..503V \| http://ui.adsabs.harvard.edu/#abs/2008AdSpR..41..503V 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	2017-03-31T05:14:04Z/2017-04-01T04:50:44Z
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	2018-04-20T22:00:00Z
Last Update	2025-01-27
Keywords	"magnetospheric structure", "perform broadband", "emission structure", "brightest magnetar", "phase dependent spectral", "1e 1841 045", "data set", "NuSTAR", "surface temperature", "magnetic field topology"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Ersin Gogus, 2018, 'Mapping the Emission Structure of the Brightest Magnetar, 1E 1841-045', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-caov8zy