A dataset provided by the European Space Agency

Name: Joint XMM-NuSTAR Observations of 1E 1048.1-5937
Published: 2014-08-31T00:00:00Z

Proposal ID	072333
Title	Joint XMM-NuSTAR Observations of 1E 1048.1-5937
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723330101
DOI	https://doi.org/10.5270/esa-em3abra
Principal Investigator, PI	Dr Victoria Kaspi
Abstract	Hard X-ray emission from magnetars was discovered by INTEGRAL, and generallycomprises more luminosity than is seen below 10 keV. However, the origin of thispowerful hard X-ray emission is unknown. NuSTAR is a recently launched NASAmission, the first focusing hard X-ray telescope. Operating in the 3-79 keVband, it has sensitivity ~100x better than previous telescopes in this energyrange. NuSTAR is a superb instrument for studying the hard X-ray emission frommagnetars. Here we propose simultaneous XMM and NuSTAR observations of magnetar1E 1048.1-5937, to obtain high-quality broadband X-ray spectrum to test aproposed correlation between spectral turnover and magnetic field, and forcomparison with the predictions of a new model for magnetar hard X-ray emission.
Publications	X-Ray Perspective of the Twisted Magnetospheres of Magnetars \|Weng Shan-Shan Gogus Ersin et al. \| ApJ \| 805-81 \| 2015 \| 2015ApJ...805...81W \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...805...81W Broadband X-Ray Spectral Investigations of Magnetars 4U 0142+61 1E 1841--045 1E 2259+586 AND 1E 1048.1-5937 \|Weng Shan-Shan Gogus Ersin \| ApJ \| 815-15 \| 2015 \| 2015ApJ...815...15W \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...815...15W 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 NuSTAR Observations of Magnetar 1E 1048.1-5937 \|Yang C. Archibald R. F. et al. \| ApJ \| 831-80 \| 2016 \| 2016ApJ...831...80Y \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...831...80Y Systematic study of magnetar outbursts \|Coti Zelati Francesco Rea Nanda et al. \| MNRAS \| 474-961 \| 2018 \| 2018MNRAS.474..961C \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.474..961C X-Ray Observations of Magnetar SGR 0501+4516 from Outburst to Quiescence \|Mong Y.-L. Ng C.-Y. \| ApJ \| 852-86 \| 2018 \| 2018ApJ...852...86M \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...852...86M 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	2013-07-22T15:50:44Z/2013-07-23T13:42:24Z
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	2014-08-31T00:00:00Z
Last Update	2025-01-27
Keywords	"magnetic field", "energy range", "hard xray emission", "launched nasa mission", "magnetar 1e 1048", "1e 1048", "spectral turnover", "NuSTAR", "superb instrument", "XMM", "79 kev band"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Victoria Kaspi, 2014, 'Joint XMM-NuSTAR Observations of 1E 1048.1-5937', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-em3abra