A dataset provided by the European Space Agency

Name: Final measure of the dipolar magnetic field of the first low-B SGR
Published: 2013-09-12T00:00:00Z

Proposal ID	069310
Title	Final measure of the dipolar magnetic field of the first low-B SGR
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693100101
DOI	https://doi.org/10.5270/esa-0221ybq
Principal Investigator, PI	Dr Nanda Rea
Abstract	We have recently discovered the first SGR with a low magnetic field (Rea et al.2010, Science, 330, 944), SGR 0418+5729, discovered in outburst after it emittedbursts similar to those of magnetars (B<7.5x10^{12} G). This discovery had largeimplications not only for the magnetar model, but for the pulsars population ingeneral. We have now a tentative measure (at 2.8sigma level) of its periodderivative resulting in a B-field =7.1x10^{12} G). We ask now for a final 75ksXMM observation to confirm this detection at >5sigma. This will lead to have afinal measure of SGR 0418+5729 dipolar magnetic field, crucial for tuning themagnetar model as well as predict how many hidden magnetars there might bewithin the pulsar population.
Publications	The Outburst Decay of the Low Magnetic Field Magnetar SGR 0418+5729 \|Rea N. Israel G. L. et al. \| ApJ \| 770-65 \| 2013 \| 2013ApJ...770...65R \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...770...65R Unifying the observational diversity of isolated neutron stars via magneto-thermal evolution models \|Vigano D. Rea N. et al. \| MNRAS \| 434-123 \| 2013 \| 2013MNRAS.434..123V \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.434..123V Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov V. N. \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y Modelling of the surface emission of the low magnetic field magnetar SGR 0418+5729 \|Guillot S. Perna R. et al. \| MNRAS \| 452-3357 \| 2015 \| 2015MNRAS.452.3357G \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.452.3357G Magnetic fields in neutron stars \|Vigano Daniele \| PhDT \| 0-7 \| 2013 \| 2013PhDT.........7V \| http://ui.adsabs.harvard.edu/#abs/2013PhDT.........7V 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 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 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 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 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	2012-08-25T14:18:08Z/2012-08-26T12:02:07Z
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	2013-09-12T00:00:00Z
Last Update	2025-01-27
Keywords	"pulsar population", "period derivative", "5x10 ^{", "SGR 0418+5729", "8sigma level", "emitted bursts", "1x10 ^{", "final 75 xmm", "magnetar model", "sgr 0418", "dipolar magnetic field", "XMM", "pulsars population"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Nanda Rea, 2013, 'Final measure of the dipolar magnetic field of the first low-B SGR', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-0221ybq