A dataset provided by the European Space Agency

Name: Timing the Energetic New Magnetar in HESS J1713-381 = CTB 37B
Published: 2013-04-04T00:00:00Z

Proposal ID	067033
Title	Timing the Energetic New Magnetar in HESS J1713-381 = CTB 37B
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670330101
DOI	https://doi.org/10.5270/esa-xxd6dv2
Principal Investigator, PI	Prof JULES HALPERN
Abstract	The spin-down power of the 3.82 s pulsar in the SNR CTB 37B is among the largestof magnetars. In addition, its spin-down rate increased by a factor of 2 thisyear. We propose to continue to monitor its spin-down. Magnetars with thelargest spin-down torque are SGRs, and a marked increase in their spin-down rateoften precedes an outburst. In this regard, CXOU J171405.7-381031 is verysimilar to SGR/AXP 1E 1547.0-5408, the magnetar with the largest spin-downpower. By analogy with 1E 1547.0-5408, we may be observing the behavior of amagnetar just before it becomes an SGR. Continued study of its spin-down willalso enable us to evaluate whether the magnetar can contribute to the TeVemission from HESS J1713-381, in which it resides.
Publications	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 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 A systematic study of soft X-ray pulse profiles of magnetars in quiescence \|Hu Chin-Ping Ng C.-Y. \| MNRAS \| 485-4274 \| 2019 \| 2019MNRAS.485.4274H \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.485.4274H XMM-Newton spectrum of the magnetar CXOU J171405.7-381031 \|Watanabe Haruka Bamba Aya et al. \| PASJ \| 71-84 \| 2019 \| 2019PASJ...71...84W \| http://ui.adsabs.harvard.edu/#abs/2019PASJ...71...84W X-ray and radio studies of SNR CTB 37B hosting the magnetar CXOU J171405.7-381031 \|Blumer Harsha Safi-Harb Samar et al. \| MNRAS \| 487-5019 \| 2019 \| 2019MNRAS.487.5019B \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.487.5019B X-Ray Monitoring of the Magnetar CXOU J171405.7-381031 in Supernova Remnant CTB 37B \|Gotthelf E. V. Halpern J. P. et al. \| ApJ \| 882-173 \| 2019 \| 2019ApJ...882..173G \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...882..173G 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 EXTraS project: Exploring the X-ray transient and variable sky \|De Luca A. Salvaterra R. et al. \| A&A \| 650-167 \| 2021 \| 2021A&A...650A.167D \| http://ui.adsabs.harvard.edu/#abs/2021A&A...650A.167D 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	2012-03-13T10:41:01Z/2012-03-13T15:22:57Z
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	2013-04-04T00:00:00Z
Last Update	2025-01-27
Keywords	"ctb 37b", "tev emission", "axp 1e 1547", "cxou j171405", "1e 1547", "rate increased", "HESS", "hess j1713 381"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof JULES HALPERN, 2013, 'Timing the Energetic New Magnetar in HESS J1713-381 = CTB 37B', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-xxd6dv2