A dataset provided by the European Space Agency

Name: HARD X-RAY TIMING BEHAVIORS OF MAGNETAR ACTIVITIES:TOROIDAL FIELD IN SGR 1900+14
Published: 2017-11-11T23:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	079061
Title	HARD X-RAY TIMING BEHAVIORS OF MAGNETAR ACTIVITIES:TOROIDAL FIELD IN SGR 1900+14
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0790610101
DOI	https://doi.org/10.5270/esa-vleqjzy
Principal Investigator, PI	Dr TERUAKI ENOTO
Abstract	The non-thermal hard X-rays of magnetars are a crucial key to understand theirmagnetic activities,or even a unique way to access the toroidal magnetic fieldhidden inside a stelar interior. A new signature of stellar free precision hasbeen suggested from two sources 4U 0142+61 and 1E 1547.0-5408. This can beinterpreted as a distortion of stellar shape due to the extremely strongtoroidal field of magnetars. However, the results are only limited to Suzakuobservations from a few sources. It is hence imperative to confirm whether sucha signature does exists in other magnetars from NuSTAR observations. We proposea 120 ks observation of a prolific soft gamma repeater SGR 1900+14 which hardX-ray timing and spectral nature has yet to be investigated in detail.
Publications	Temporal and spectral X-ray properties of magnetar SGR 1900+14 derived from observations with NuSTAR and XMM-Newton \|Tamba Tsubasa Bamba Aya et al. \| PASJ \| 71-90 \| 2019 \| 2019PASJ...71...90T \| http://ui.adsabs.harvard.edu/#abs/2019PASJ...71...90T 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 Magnetars and axion-like particles: probes with the hard X-ray spectrum \|Fortin Jean-Franu00e7ois Guo Huai-Ke et al. \| JCAP \| 6-36 \| 2021 \| 2021JCAP...06..036F \| http://ui.adsabs.harvard.edu/#abs/2021JCAP...06..036F Discovery of 40.5 ks Hard X-Ray Pulse-phase Modulations from SGR 1900+14 \|Makishima K. Tamba T. et al. \| ApJ \| 923-63 \| 2021 \| 2021ApJ...923...63M \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...923...63M Correlation Study of Temporal and Emission Properties of Quiescent Magnetars \|Seo Jiwoo Lee Jaewon \| JKAS \| 56-41 \| 2023 \| 2023JKAS...56...41S \| http://ui.adsabs.harvard.edu/#abs/2023JKAS...56...41S The common fundamental plane of X-ray emissions from pulsars and magnetars in quiescence \|Chu Che-Yen Chang Hsiang-Kuang \| MNRAS \| 526-1287 \| 2023 \| 2023MNRAS.526.1287C \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.526.1287C 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 New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2016-10-20T21:43:05Z/2016-10-21T04:06:25Z
Version	21.51_20241115_1113
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	2017-11-11T23:00:00Z
Last Update	2026-06-19
Keywords	"stelar interior", "stellar free precision", "hard xray", "nonthermal hard xray", "SGR 1900+14", "magnetar activities", "toroidal field", "NuSTAR", "magnetic activities", "sgr 1900", "1e 1547", "sources 4u 0142", "stellar shape"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr TERUAKI ENOTO, 2017, 'HARD X-RAY TIMING BEHAVIORS OF MAGNETAR ACTIVITIES:TOROIDAL FIELD IN SGR 1900+14', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-vleqjzy
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.