A dataset provided by the European Space Agency

Name: Final measure of the dipolar magnetic field of the first low-B SGR
Published: 2014-09-07T00:00:00Z

Proposal ID	072381
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=0723810101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723810201
DOI	https://doi.org/10.5270/esa-yk5gnuu
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 3.5sigma level) of its periodderivative resulting in a B-field virgul6x10^{12} G). We ask now for a final 75ks XMMobservation to confirm this detection at >5sigma. This will lead to have a finalmeasure of SGR 0418+5729 dipolar magnetic field, crucial for tuning the magnetarmodel as well as predict how many hidden magnetars there might be within thepulsar population.
Publications	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 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 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 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 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	2013-08-15T18:06:25Z/2013-08-18T11:57:17Z
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	2014-09-07T00:00:00Z
Keywords	"period derivative", "emitted bursts", "XMM", "5sigma level", "SGR 0418+5729", "final 75 xmm", "6x10 ^{", "5x10 ^{", "magnetar model", "sgr 0418", "pulsar population", "dipolar magnetic field", "pulsars population"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Nanda Rea, 2014, '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-yk5gnuu